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subset: commoncrawl


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Nationally recognized immigrant rights leader Ravi Ragbir was detained today, while reporting to Immigration and Customs Enforcement for a routine check-in.
The sudden arrest of the Trinidadian-born migrant, whose legal status - like many migrants - has been in a state of limbo for nearly ten years, sparked demonstrations outside the Manhattan federal building where he is being held.
Reverend Dr. Donna Schaper of Judson Memorial Church said that the city and the nation would be much worse off if Ragbir were to be deported.
Ragbir has been facing the threat of deportation for almost a decade, community members said, due to a "16-year-old conviction for wire fraud". He is now executive director of the New Sanctuary Coalition.
SAALT and other organizations have started a massive campaign to get Ragbir released from ICE detention, asking community members to call the offices of Sens.
In a statement late Thursday, an ICE spokeswoman said Ragbir had "exhausted" his petitions and appeals and would be deported.
"Obviously we are incredibly disappointed and, frankly, outraged by this decision", Das told VOA. "We continue to pursue our options - the legal challenges - to see that he will hopefully be freed soon and back with his wife and with the community that loves him".
Missouri governor admits affair, accused of blackmailing woman with photo
McCann Beatty said it's unfortunate that Greitens didn't address the concerns of protesters in St. Libla is circulating a letter among his colleagues after a report on Wednesday by KMOV-TV in St.
At the time this report was published, ICE had not responded to VOA's request for comment regarding Ragbir's arrest.
Democracy Now! was there this morning when New York City police officers violently shoved protesters and city council members aside as they escorted an ambulance away from 26 Federal Plaza with Ragbir inside to an ICE detention center.
Some tense moments erupted Thursday during a rally in Lower Manhattan for undocumented immigrants facing deportation. As she spoke of Ragbir and the nationwide workplace raids, tears rolled down beneath her sunglasses.
"It is crippling for the immigrant community", Young said. "If you are here in the country and you decide to go find a job, and they're targeting your workplace, you're not a criminal".
Previously, those community members said, ICE officials had granted Ragbir "prosecutorial discretion, including a stay of removal that was in effect until next week".
"After those arrested had been removed, the remaining group of activists continued to chant in support not only of those who had been taken by the NYPD but Ravi himself", Williams said. "We're not even one bit afraid".
Trivedi told India-West that after Ragbir was released from immigration detention in 2008, he was inspired by his experiences while incarcerated to speak out on prison reform and immigrant rights.
Related articles
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5 Essential Elements For Pay Double
The Definitive Guide to Best Bitcoin Cloud Mining Website
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If The pinnacle of the agency decides that a unique "in lieu of" holiday break is necessary to stop an "adverse agency impact," they may designate a special "in lieu of" vacation for full-time workforce less than compressed function schedules. (See five U.S.C. 6131(b).)
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From publisher blurb:
Super Bad Guys! #1 for ICONS offers three new villans for your "Superpowered Roleplaying" game. Each unique bad guy includes attributes, specialties, powers, and qualities, along with a summery of their criminal creation and monsterous motives.
There can never be enough bad guys -- and neve ever enough Super Bad Guys!


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- Variable Cost
It is the cost that changes with the amount of production or the amount of work.
eg. Wages, cost of material, etc
- Fixed Cost
It is the costs that do not change as production changes.
eg. one-time setup cost, rental cost, etc
This site contains information for your preparation of PMI's PMP (Project Management Professional) certification exam. I have also Included topics on how to pass the exam and some mock exams.
Saturday, February 2, 2008
Variable and Fixed Costs
What are the difference between Variable and Fixed Cost?
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Suggested Study Materials
- PMP-Preparation Recommended Books
- PMP Exam Prep, Fifth Edition: Rita's Course in a Book for Passing the PMP Exam
- A Guide to the Project Management Body of Knowledge, Third Edition (PMBOK Guides)
- The PMP Exam: How to Pass On Your First Try (Test Prep series)


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From the PDF Introduction
A Monster Manual (D&D 3.5e) v3.5 Web Enhancement
The organization entries in the Monster Manual give some indication of what kinds of groupings various creatures might form. These entries are intended as examples to get you thinking about how the creatures live and act from day to day.
When you sit down to create an adventure or encounter featuring a group of creatures in their lair, you can use the organization entry (along with other elements of the creature description) as a creative springboard.
The sample lair presented here is an outpost used by a hobgoblin war party. It also embodies some elements of a hobgoblin tribal lair.


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After hearing much buzz about The Odin Project, I decided to check it out. Part of my personal learning while I'm here at Harvard is to build skills that will make me more hirable. I'm still exploring possible career paths but generally, most of the things I'm interested require a better understanding and familiarity with the technical side of things.
The Odin Project is a free self-paced course on web development. This is from their site and explains their project:
I think that's a pretty cool concept. I don't know exactly how many people are using this site, but I think it has the potential to be a massive space.
While not all the lesson pages have user discussions, I think it's great that on the ones that do, there's interactions and exchanges between users. I also think it's great that the site has a section on forming in-person study groups and providing resources to connect with other learners. I think it helps address the issue of isolation when learning something on your own. It's nice to be able to interact with others.
I've only explored the first section, but here's what I like:
- Simple design – everything flows really well
- The information is categorized in a logical manner with learning goals for each section
- Built in user comments/discussions
- Validation on progress
I really love this progress bar. As you go through each page, the circles fill up and you see the percentage of content you've finished looking at.
I also really like that you get to "check" each lesson as you complete it.
I'm a huge fan of the design and overall information layout.
Has anyone else tried this out?


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i was listening to them for the first time in ages today... jus sat here at the computer ....and it sounded fantastic!!
yknow once you are away from the hype and music channels playing them too much ... these are damn good songs !
yknow once you are away from the hype and music channels playing them too much ... these are damn good songs !
Re: nirvanaTo your ears maybe.
Nevermind is possibly the most overated album of all time. Nirvana aren't shit like, but they're not great either.
Re: nirvanaYeah but Nirvana fans don't rate Nevermind, on the whole.
Re: nirvanayeah, that's why i tried to ignore them so much initially ('cos of hype / over-exposure) but when Kurt's death anniversary happened last year (?) and they started playing songs other than bloody '...Teen Spirit' it was a case of 'bloody hell, these were good songs weren't they!'
so yeah.
Re: nirvanaNirvana are one of my absolute favourites.
Third band that i truly fell for...
Re: nirvanaYou do know that Lauryn Hill may eat your children...dont you?
Re: nirvanasays the ryan adams fan . . .
Re: nirvanai can never get enough of incesticide
Re: nirvanaI always thought In Utero was the best album. Then i realised it was produced by Steve Albini and found out who he was. Everything was explained.
Re: nirvanaIn Utero is grrreat but a good few songs i can't stand on it - pennyroyal tea, rape me. Bleach has its charms. i think for me now, Nirvana are a once every 3 months sorts band
Re: nirvanaLoad of shite.
If Cobain hadn't decorated the walls no one would care. Hackneyed argument I know, but true. ;-)
Re: nirvanaNirvana were adored before 1994.
Cobain is not a Nick Drake or Van Gogh.
Re: nirvanaI've always thought Pixies were more of a 'hooks' band while Nirvana are more about 'tunes'.
I love In Utero, but I like all the albums really.


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Sound View Commission Minutes 02/28/2017
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Sound View Commission
Meeting Minutes — Unapproved
28th February, 2017
7.30 pm
Town Hall Meeting Room
Present: Frank Pappalardo (Chair), David Kelsey, Joann Reis Lishing, Michaelle Pearson (Secretary), Jackie Miano (Alternate), Sandra Ziemba (alternate)
Also Present: First Selectwoman Bonnie Reemsnyder, Selectwoman Mary Jo Nosal,
Absent: Harry Plaut, Frank Maratta (Alternate),
7.32 pm Meeting called to order
by Chairman Frank Pappalardo.
Alternate Sandra Ziemba seated for the absent Harry Plaut
Approval of January Minutes:
Joann Lishing motioned to approve, David Kelsey seconded. All in favor. Minutes approved.
7.34pm: Miami Beach Fence Update (First Selectwoman Reemsnyder)
First Selectwoman Bonnie Reemsnyder said that the Board of Selectmen had received a lot of comments regarding the fence. She spoke with the town attorney to determine if the town has jurisdiction. She also reached out to DEEP, as the fence appears to reach past the Coastal Jurisdiction Line and past the High Water Line; and the Office of Long Island Sound Programs (OLISP), because the fence will limit access. Waiting for final determination. The First Selectwoman also contacted the Connecticut Attorney General's office. They said the case from the 1950s was brought by "The People" not by the town. Hence, the town attorney did not feel that the town had jurisdiction. The "people" do. Anyone who feels their rights are abridged has a right to bring a lawsuit. Best standing for a case would be brought by descendants of the original people who filed the case, or successors to their property.
Mrs. Reemsnyder explained that the town gives stipends to private beach associations to support their effort on security. White Sands (a town beach in a private association) and Miami Beach (public access from Sound View) receive approximately an extra 10K per year (over what other beaches receive) according to formula. If MBA is collecting money and controlling access, is the impact the same? She said the BOS had an extensive conversation with Miami Beach. This is a pilot program. MBA may not make enough money to cover their security. They are receiving public funds, as are all the other beaches. The BOS will need to look at this carefully. We could look at it and see what happens this summer.
Jackie Miano said that she thought it best to let it happen for a year and evaluate the results.
Frank Pappalardo expressed concern that this may place stress on town resources. The Rangers will be checking coolers, but some of those people will go to Miami. That burden may need to shift.
Mrs. Reemsnyder said that Miami Beach Association promised to get back to the Board of Selectmen by mid-March regarding any detailed plans. This may be an ongoing conversation for the coming year.
Frank Pappalardo said that Miami was very clear about allowing access to Sound View residents and Old Lyme residents.
Jason Matarazzo, Portland Ave., asked if MBA receives an extra 10K over other beaches, why doesn't the town suggest they use that to fund security guards? Mrs. Reemsnyder explained that the money is funded based on what the beaches spend each year on security. Only up to 50% of the cost. No beach is reimbursed more than 50% of their expense for security.
Frank Pappalardo said that this year Miami is looking at a higher-caliber security firm. Better level of protection, including night security. Beach stipend committee has the formula on town website.
Stephanie Livesey, Swan Ave., asked if this means the town could be paying more for MBA security in the future?
Mrs. Reemsnyder reiterated that there is a limit. Because MBA has been open to the unorganized general public, the town has acknowledged that beach is disproportionately affected by Sound View parking spaces.
Angelo Faenza, Portland Ave., said he hopes they would come to some conclusion as far as residents are concerned. Might want to take a look at that court case.
Lenny Corto, Jr., of Lenny's on the Beach, Hartford, Ave., asked if because Miami is charging money, isn't that a change of use to revenue/ commercial? Doesn't that change their zoning status? Mrs. Reemsnyder said there may be tax implications there. They may have to charge tax.
Jason Materazzo asked about passes for renters, or extended family groups, kids/ grandkids? Frank Pappalardo agreed that was a good question. Miami Beach will have to make some accommodation or there will be a lot of upset people. Not sure how they will handle that.
7.59 SVIC Update.
Met last week re: Hartford Avenue drainage. Pipe that no one knew existed down Martino between Hartford and Portland. Meeting held on site and WMC & BSC are looking at it to ensure that it won't adversely be affected.
Sandra Ziemba asked if this would affect the timeline. Frank Pappalardo said it shouldn't, as this doesn't appear to be a major construction issue. Time and money have been figured into the initial cost. Work is on hold for the winter. Target for completion is still early May. Expansion joints are also under review by Ed Adanti and BSC.
Selectwoman Nosal added that the engineers met on Friday, and will have another meeting to get revised cost estimate for the drainage going forward.
2016 Summer Evaluation Update:
Received some statistics. Attached. Still would like to see further info that should be readily available from kiosk data to clarify the picture, such as parking stats, etc.
Mr. Pappalardo has some questions from residents to present to new state trooper, re: Community policing, etc.
David Kelsey suggested a survey for residents re their experience each summer. Very simple, and restricting it to the primary issues.
Jason Materazzo asked how much money do Rangers cost vs. troopers, and what are Rangers' responsibilities.
Frank Pappalardo said the Rangers perform cooler checks and write parking tickets.
Resident Trooper Status:
Target date is 4/1/17. There are also vacancies for 2 Old Lyme Police Officers.
Angelo Faenza expressed concern as to how the new bill before the State legislature might affect us…100% plus 750 per officer.
Mrs. Reemsnyder said it's concerning, but not as much as the teacher retirements. The Selectmen are currently considering 2 troopers, 4 cops; or 1 trooper, 6 cops. Board of Selectmen working on calculation. Frank Pappalardo said the goal is to increase staffing levels so we have adequate coverage on weekends. We did not have adequate coverage last year.
Zoning Board of Appeals Variance Approvals Information:
Some questions raised at last meeting regarding Cool Moose variances granted. Case: 16-06, March 2016. Variances granted for moving package store to another location and change of use from commercial to residential. Building and zoning permits needed, but none filed for 61 Hartford Ave.
The Permit is solely for replacement of roof and siding not for changing configuration of building. No Zoning Commission approval. The DiNinos received a letter stating they must apply for the proper zoning and building permits. They also changed the roofline which increased the footprint. According to Zoning Enforcement Officer Keith Rosenfeld they have not received a building permit or zoning approval.
Sons of Italy Hall/ 280 Shore Rd.:
New owners have zoning variances for parking buffers. Proposed professional office, gambrel style, same footprint. Owner occupied. Dentist office, Lawyer office. Frank Pappalardo looked at the plans and thought the variances made sense. Main entrance on Rte. 156. Side entrance for employee-only parking on side of Portland Avenue. Owners will put up a gate /chain to prevent beach parking. Next month they will go to zoning with their site plan, mechanicals and safety plan.
Osprey Festival:
Very successful last year. People wanted festival to be closer to the water. Mark Griswold (Chairman Chamber of Commerce) asked if it could be in the town lot. A draft plan was developed by Frank Pappalardo as requested by Mr. Griswold. Date of the festival is June 17th. Lot will be closed for the day. Hours reduced: 10am-6pm.
Michaelle Pearson asked where festival-goers will park. Frank Pappalardo said there will be temporary, one-day only permits issued to Gail's green, church and maybe one other. Parking across from PD.
Shuttle bus parking lot? Designated drop off for bus. Possible golf cart to shuttle vendors and entertainers.
At the March 6th Selectmen's meeting, the Board of Selectmen will be reviewing all the Osprey festival plans.
SVBA pancake breakfast same day. Also coffee and pastries in afternoon.
8.48pm: Parking Lot Sub-Committee Update (Sandy Ziemba):
Jen Lathrop, Sandy Ziemba, Harry Plaut, Bob Tonon. Have reached out to Miami Beach as well. Would like a Miami beach resident to be on this committee.
Met 1/31. FP, Jen Vowles, Bob Tonon, Sandy. Discussion and recommendations of subcommittee:
Concerns with lack of enforcement. Printed out a questionnaire so committee can make recommendations to SVC. Discussion of ordinance 161-2.
Parking in unpermitted lots is an ongoing problem. How will the MBA fence impact the parking situation? Will towing be reinstated?
What about issues after-hours? The lot permits are from 9am-6pm, but there's nothing in the regulations to ask people to close.
$100 for each violation for cars above permit. $100 day for subsequent violations. Unpermitted lots $500, plus $1000K
Should private parking lots be required to have insurance? For how much?
Brief discussion as to how owners can handle unruly individuals. Lot owners feel that they should have backup and be able to call police for help in these situations.
Public/ unattended lots, activities on town beach. Need more enforcement.
Would like town to subcontract a tow truck to handle some of these illegal parking issues. From 2012-14 there was significant towing of illegally parked cars. Might look at re-establishing this. Sub-committee will meet again soon.
Angelo Faenza stated that most of these are zoning issues. That's been a problem for years. Zoning doesn't work on Sunday. Need someone to be responsible for this. Who monitors the lots? Rangers?
Events Sub-Committee:
Will meet soon to plan summer activities.
SVVD Sub-Committee:
David Kelsey said last developments were in September. Frank & Dave Noe were going to provide renderings and their site plan. Haven't heard from them since then. Dave will
contact them re any further developments.
Other Business: Board of Selectmen is looking into obtaining video cameras for the town lot and Hartford Avenue.
Public Comment:
Joe Tulisano, Hartford Avenue, asked what happened with the Historical District designation?
Frank Pappalardo reported that Sound View has been recognized as a State Historic District, and is on the Connecticut State Register of Historic Districts. There has not yet been a determination regarding the National Historic designation, as that comes from National Parks. The application is pending, though it might be a long wait, due to funding cuts.
Mr. Tulisano also asked if the new Hartford Avenue sidewalk was indeed 6 feet wide, because it looked smaller? Frank Pappalardo and the Selectwomen said that it had been measured and was in fact 6 feet.
Lenny Corto, Jr asked if the plan was on time to be completed before Memorial Day, and also if the lot will be reconfigured. Frank Pappalardo said the town lot will have a single entrance/exit. Will be reconfigured in time for the season. There will be designated parking for town residents in the lot, as there always has been.
9.22pm: Adjournment:
Joann Lishing motioned to adjourn. Sandy seconded. All in favor. Motion carried.
Meeting adjourned at 9.22 pm.
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Parker Wheeler Joins The UNH Men's Hockey Blog
I'm excited to announce that Parker Wheeler, the play-by-play broadcaster of UNH men's hockey for WUNH 91.3 FM, has accepted my invitation to write for The UNH Men's Hockey Blog. Beginning with the Wildcats' exhibition game against St. Francis Xavier University, Parker will share his observations and analysis in an ongoing series of game reports.
Parker Wheeler, a UNH senior majoring in Kinesiology with a minor in Journalism, is the Sports Director of the WUNH Sports Department. This season marks his second as the play-by-play announcer of men's hockey. Parker is the on-air host of Wildchats, the Thursday night pregame show from 6-8 PM on WUNH. He is also the play-by-play broadcaster of UNH women's soccer, volleyball, and field hockey for America East TV.
In addition to Parker's extensive knowledge of the UNH hockey program, he's an accomplished player in his own right. He was a goaltender for four years at ConVal Regional High School in Peterborough, NH. In his final two seasons, he was ConVal's starting goalie and was named the First Team All-State goalie for New Hampshire High School Division III in his senior year.
After four seasons of covering all UNH hockey home games and many away games, I'm looking forward to handing the reins over to a student journalist who possesses a unique combination of passion, experience, and insight. I will continue to report on the progress of the team but in a different role. I'm developing a new feature for The UNH Men's Hockey Blog which will begin with the regular season opener against American International College. Stay tuned.


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This post will only be of interest to people who live in the U.S. and have longed for the Greek "chorta" salad. I finally, FINALLY, found the leafy green vegetable which can make a decent "chorta" salad. "Chorta" salad in Greece means greens cooked in water and served with salt, olive oil and lemon. There's some variety of Greek greens that make nice "chorta'" salads but my favorite are the ones ones with crunchier or more "wild" textures. The verdict is out. Drum roll, drum roll, drum roll. The American vegetable that's closest to the desired taste and texture is … the curly endives variety of chicory greens! They are sturdy enough to remain crunchy after cooking and have this bitter flavor that I love. I followed the same cooking method as for "chorta", i.e., boil in water until soft, add salt, pepper, plenty of olive oil and lemon. Before serving, I added two big cloves of garlic for flavor. I wouldn't eat the cloves but they did a great job giving a little extra "kick" to the salad.
Cooked chicory salad with garlic


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by Teresa Peterson
Greetings CineSportsTalk fans, allow me to introduce myself, I'm Teresa Bellomo Peterson aka The Gossip Whore. My hubby, cofounder here (I'll let you guess which one) has been harassing the crap out of me to write a gossip column. He seems to think that just cause I have more frenimies that any woman he has ever met, and I trash talk anyone and everyone, I may be on to something here. So like it or not here I am ready to give you the low down on the low down and talk some trash about anyone I deem suitable, which pertains to pretty much everyone….(family members not discluded) First up is my girl Bethenny. Looks as though her marriage is over, sigh. Shocker? Not so much. I actually really like Bethenny, she reminds me of myself, other than the fact that she weights 80 lbs soaking wet and is a millionaire, we have many things in common. She always blurts out what's on her mind and she is extremely abrasive, a quality I take crap for at home and in the office. Sorry but if we were men it would be perfectly fine to be obnoxious, abrasive and painfully honest. But nope instead we should know our role! Well I applaud Bethenny for getting where she is today by being who she is. Bravo Bethenny (get the pun) Her marriage however was doomed from the start. I have watched her since RHNYC when she was single. I get that she wants to be herself. But when she chose this poor schmuck I knew he was doomed. He is way too much of a yes man. Stand up for yourself man, where are your balls?? Bethenny, I get you, I really do. But sometimes you have to play the pretty dumb girl (bats eye lashes, wink wink) Let him think he is in control. Think is the operative word here. It was painful to watch her with is family, ouch! If I have learned anything being married its play nice with the family, just smile, nod and keep your mouth shut. Remember they don't really consider you family anyhow. They just tolerate you and don't care about your opinion. Poor Jason had no idea what he was getting himself into. My advice to Jason, RUN and don't forget to grab half her millions from her Skinny Girl account.
On to breaking news Kim Kardasian changed her hair color back to black!! Gasp! Well it looks like Jessica Simpson wont be fitting into her daisy dukes again for quite a while as she's preggers again. Damn she didn't waste one minute going back for seconds. Good for her cause I'm pretty sure poppy out babies is the only talent she has. I am so annoyed by this next couple I was not even going to mention it. Katy, Katy, Katy bringing John Mayor home to meet the parents for Christmas, really? I guess after Russell dumped you publicly you thought it was a bright idea to date the second worst man whore around after Russell? I was rooting for you after he left. We all make mistakes, we have all dated the bad guy but some girls are just asking for it. Katy now that your teenage dreams have been shattered get ready to start singing Love is a Battlefield. And last but not least Kate Winslet was secretly married to a man whose last name is, wait for it, Rocknroll?! I have no idea who he is other than the nephew of billionaire Richard Branson. So he is basically nobody who wants to be somebody so he changed his name to Rocknroll dude! Not, moron. For her third walk down the aisle Leo DiCaprio gave the blushing bride away, how sweet. I guess Leo figured he might as well walk down the aisle once in his life. Seeing as how every woman he dates is a blond bim- I mean super model, and his relationships last as long as the amount of English they know. Well that's it for me I'm outta here, hope everyone has a happy new year!! See you on the other side.


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Taken at Jumeirah beach Cornish..
Thursday, 13 November 2014
Slow down
6 comments:
Useful sign or not ?ReplyDeleteReplies
it should be useful for construction vehicles. : )Delete
It looks like a complete stop my be more appropriate.ReplyDeleteReplies
: )) this is the entrance of the construction at the beach Jumeirah. I suppose the speed limit is for construction vehicles..Delete
I'm not sure I'd want to be driving on that.ReplyDeleteReplies
hahah I did that mistake once.. it was not easy to get out from that sand.Delete
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Lyme Disease treatment in Germany: Read all of my Infusio posts here.
Disclaimer: I went through the Integrative Lyme Disease treatment program at Infusio, Frankfurt from the 23rd October to the 3rd of November 2017. During this time, I kept a journal of my experience and I am now sharing this with you here. Please keep in mind that this is my personal experience. The treatments and therapies I had were based on what was best for me as an individual. Therefore, if you have been to Infusio, Frankfurt or are planning to go, your experience may differ from mine.
Friday 3Rd November 2017
Part of me couldn't believe it was my last day of treatment at Infusio. Having said that, I was definitely ready to go home and start healing.
Like yesterday, today it was another struggle to find a suitable vein. The veins in my arms had pretty much given up by this point! After a couple of failed attempts, Dr Bijan was asked to have a try. He took a look at my arms and decided it wasn't even worth trying there.
I had to have the IV needle inserted into a vein in my hand. They normally try to avoid doing this as it tends to be a bit painful. I was definitely more aware of having the IV in my hand but it wasn't actually too bad. Plus, I only had 2 IV's today so it wasn't in for long.
Today's IV Treatments
The IV's that I had today were:
- A mineral infusion
- Curcumin: an anti-inflammatory.
Speaking With Dr Bijan
I was relieved and happy to be finished two weeks of IVs. After they were done, I spoke to Dr Bijan about my latest blood test results. My ATP (the body's energy molecule) was still poor but this was to be expected; I found treatment to be hard-going and it would also take time for this to improve.
The good news was that my red blood cell count (RBC) had increased a little. It was now at the lower end of normal. I was pleased about this as it meant that I didn't have to take any injections home with me.
During my first consult with Dr Bijan, he had explained that I was anaemic. Due to this, I was told that I may need to take treatment home with me if my RBC didn't improve sufficiently during my time at Infusio.
This treatment would be a course of injections (the same as I was given on Day 3). The injections help to stimulate red blood cell production and treat anaemia.
I have to say, I was glad I didn't need them! The idea of self-injecting wasn't appealing.
Going Over My Latest Global Diagnostics Scan
Nadine also chatted with me about my latest Global Diagnostics scan (read about what this is here). Some things showed up as worse than in the first scan. For example, my cellular energy was lower. However, Nadine explained that this was due to the healing processes taking place in my body (which require lots of energy).
Some areas had definitely improved, though. The level of toxins and inflammation in my body had greatly decreased; which is probably why my body liked those detox IVs so much!
Organs that had shown up as red in my first scan (i.e. not working properly) were now green. This included my liver, gallbladder, pancreas and bladder. It was only my intestines that were still displaying as a problem area.
Of course, this is just the results following the first two weeks of treatment. I only had my stem cells a couple of days ago and this is when healing really begins. So, it will be interesting to see how things have changed when I go back for my follow-up appointment.
Final Treatment
My last treatment of the day was an amazing foot massage. It was so relaxing and I couldn't think of a better way to end my experience at Infusio.
I actually felt quite emotional when I had finished treatment. There was definitely a mix of emotions going on. I felt so much gratitude for being able to have this treatment. And, I also felt an immense appreciation for Dr Bijan and all of the Infusio team.
But, I also felt a little sad. I guess it's always sad to say goodbye to people who you have spent time with. Especially, when that time is spent doing something so profound and life-changing. The team at Infusio are all so wonderful and I was lucky to have gone through this experience with a great group of people.
Our group finished with a healing hug, then it was time to leave. I left Infusio feeling good, joyful and incredibly grateful.
Read Next: My 4 week post stem cells update
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Lyme Disease treatment in Germany: Read all of my Infusio posts here.


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EDGEFIELD, S.C. – The National Wild Turkey Federation knows turkey hunters demand the best gear possible from reputable companies when it comes to their spring pursuits, and a new long-term partnership with Plano Synergy and their turkey brands shows the NWTF is committed to backing quality products.
Effective November 1, Avian-X and Zink Calls are the official turkey decoy and call of the NWTF, respectively.
"The NWTF is pleased to align with Plano Synergy and its turkey-hunting brands," said NWTF CEO, George Thornton. "They are known for creating innovative and high-quality products, sharing our core values, supporting our mission and are committed to the efforts to Save the Habitat. Save the Hunt."
Details of the partnership with Plano Synergy include, but are not limited to:
- Avian-X and Zink Calls will bear the NWTF logo and title of official products of the NWTF on respective packaging.
- Flextone also will be recognized as an official partner of the NWTF.
- Avian-X, Zink Calls and Flextone will sponsor the Waterin' Hole at the NWTF Convention and Sport Show, February 15-19, 2017 in Nashville, Tennessee.
- Plano Synergy will be recognized in signage as a sponsor of the NWTF Hunting Heritage Center located in Edgefield, South Carolina.
"Plano Synergy is grateful for this unique partnership with the NWTF and the opportunity to play an active role in supporting its conservation mission," said Pete Angle, vice president of marketing for Plano Synergy. "The NWTF's varied grassroots programs and initiatives have educated millions of hunters and non-hunters alike on the critical importance of wildlife conservation and habitat restoration."
About Save the Habitat. Save the Hunt.
The NWTF Save the Habitat. Save the Hunt. initiative is a charge that mobilizes science, fundraising and devoted volunteers to give the NWTF more energy and purpose than ever. Through this national initiative, the NWTF has committed to raising $1.2 billion to conserve or enhance more than 4 million acres of essential upland wildlife habitat, recruit at least 1.5 million hunters and open access to 500,000 acres for hunting, shooting and outdoor enjoyment. Without hunters, there will be no wildlife or habitat. The NWTF is determined to Save the Habitat. Save the Hunt.
About Plano Synergy
Plano Synergy's foundation is built on an unrelenting passion for the outdoors. It's the very same passion we share with our customers, and why each and every product within our family of trusted high-performance brands is carefully conceived, designed and manufactured to elevate the outdoors experience. No matter how advanced or basic the need, Plano Synergy delivers hunters, anglers and outdoor-lifestyle enthusiasts the specific products that maximize the satisfaction earned from a day – or a lifetime of seasons – in the field or on the water.
For more information, contact Peter Muller at (803) 637-7698.


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"I think if you look at previous year, people might say they did or didn't, but I think they didn't want the number one seed for a reason because we would've played them in the second round", Wall told ESPN's Rachel Nichols and Paul Pierce, referring to Cleveland. "I think they didn't want that number one seed for a reason, because we would have played them in the second round".
"I think [the Cavs] understand what we can bring to the table", Wall said.
The Wizards were the #4 seed, and they pushed the Celtics to seven games in the Eastern Conference finals.
Prior to Friday night's matchup against the Cleveland Cavaliers, Bradley Beal told ESPN's The Jump, that the Washington Wizards are the best team in the East. Everybody was playing. It's not like Bron [LeBron James] didn't play, Ky [Kyrie Irving] didn't play, Kev [Kevin Love] didn't play, like we were resting guys.
"He is as tough of a competitor I've ever been around", Wizards coach Scott Brooks said. "Everybody was playing. We just had a bad rut like we just did [this season]".More news: Lebanese prime minister resigns amid tensions with Hezbollah
More news: Blistering Munro ton helps New Zealand to level series against India
More news: Asked if DNC system was rigged in Clinton's favor, Warren says 'yes'
Added Wall: "We feel like we're their biggest threat". I'm not going to sit here and do that. We know we can challenge them, and they know they challenge us.
John Wall, who's part of the MVP conversation, is averaging 21.6 points per game.
"He had an awesome game, but at the same time, we got to respect what he does and what he brings to the game".
Wall and Beal, though, don't lack for confidence, nor should they. Whenever we have lapses against those teams we should beat, it's because we don't get off to a great start.
If you come at the king, you best not miss. As a result he is listed as questionable for Washington's game against the Toronto Raptors Sunday night.


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Merry Christmas, snow bunnies! I'm dropping in for early holiday wishes today because after working like a crazy person for several months, I have finally given myself permission to step back, relax and just breathe.
So that means I will be a bit quieter in the internet world. No blog posts until after the New Year and not so much twittering and Facebooking.
The shop will remain open and I will continue to ship orders on a regular basis.
This holiday season has just worn me down so I'm taking a bit of time to think and plan and read books and watch movies and play with the pup in the snow.
But I'll also be taking the time to explore some new ideas for the shop, work on finishing some freelance projects, give the blog a little facelift and make business plans for the coming year.
I'm so excited by some of the things that will be happening in 2010 and am very curious about what other surprises the year will bring me. I hope to be sharing lots of good news!
I'll be returning to the blog year on January 1st with a fun new opportunity to share with you. Here's a hint: I might have thing or two to teach you ;)
Wishing you all the best on through the holidays and can't wait to be back for the new year!


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THE PHONE RINGS. Larry Flynt's Hustler magazine wants me for a Q&A (not T&A) about all things propaganda. The editor is familiar with my books, knows me as a critic of the Bush propaganda machine.
I've been a propaganda scholar since before it was cool (pre-9/11), trudging along in the academic trenches after a stint with the now-defunct U.S. Information Agency during the Clinton years. Hustler wants me to deconstruct political and corporate images in lay terms, somewhere between People and the Nation. I jump at any chance to explain to Americans how to view advertising and public relations of all stripes with a critical eye. But in Hustler?
The porn mag pitches its appeal with a purr. Previously it had published interviews with Jesse Jackson, Christopher Hitchens, Noam Chomsky, Greg Palast and, most recently, David Horowitz. Readership is in the millions, its staffers claim, including lots of U.S. soldiers in Iraq. How could I turn down an opportunity to explain how propaganda is the primer paint for nations going to war? I phone Mom.
Mom lives in a retirement community in the Bible Belt. She asks me to send my books for its library to prove to the other octogenarians that her daughter is a published author. Using my light-and-airy upturned-mouth voice, I say, "Hey Mom, Hustler wants to interview me about my propaganda work. Isn't that great?" I force her into a psychological corner as only daughters know how to do.


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The Living Miracles Peer Empowerment Center Board of Directors
Alberto Martir, CPS-MH, Board Chair
Certified Peer Supporter for United Healthcare/Optum Behavioral Solutions
Alberto is interested in supporting and developing peer support and the recovery model through his skills and experience as a certified peer supporter and mental health advocate. Alberto believes that Living Miracles has the potential for the further push to the paradigm shift of people helping people as peers and as part of the community, Living Miracles is a flagship for the greater advocacy of peer recovery, iconoclastic against stigma and its beliefs, and a leader towards the greater good of people in recovery.
Terri Miller, Vice Chair
Family and Consumer Support Coordinator for NAMI Greater Cleveland
Terri has worked for NAMI Greater Cleveland for over 13 years and is a mother of an individual with a mental illness, as well as having suffered from depression herself. Terri believes the importance of peer support is a crucial part of recovery. Terri is interested in furthering the mission of The Living Miracles, helping with fundraisers, community events and providing public relations. Terri would like to see the organization continue to grow, and would like to see peer support services accepted as an addition to other services provided for and by people with a mental health diagnosis.
Lee Ann Gramuglia, Director
Lee Ann is a retired Registered Nurse, and has been a member of The Living Miracles since 2009, and has also provided peer support and mentoring services to patients at Northcoast Behavioral Healthcare and The Sricklin Crisis Stabilization Unit. Lee Ann is excited to be on the Board of Directors and has a strong belief in the healing power of peer empowerment. Lee Ann would like to let others know how beneficial peer support can be.
Cheryl Lydston, LISW-S, Director
Care Manager for United Healthcare/Optum Behavioral Solutions
With over 25 years of experience working in the mental health and addiction field, Cheryl is a compassionate and tireless advocate for people with mental illness and addictions. Cheryl is excited to be on the Board of Directors and is looking forward to assisting the agency with program development, expanding the agencys funding streams and services throughout the community.


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Above all else, even your dress,and add-ons,the best formal hair do will say: You appear absolutelyfabulous! Learn just two characteristics regarding your facialfeatures and you'll no more have trouble locating the perfect hair do, for promenade, homecoming or most occasions.
Present day poor and loose dress codes and hair styles certainly possess a devote society. But, you will find occasions and occasions nowadays which show, a minimum of that formal hair styles are in route back. Lots of people have started to conclude that particular occasions or occasions do indeed require better clothing along with a good hair do.
Be versatile if this involves hair styles. We all know that formal dinner occasions will always be in fashion. Also, then, ought to be the formal hair do. People of any age today appear to become getting that, that is a welcome sign. And who does not wish to attend some kind of formal affair at least one time within their lifetime? Places or occasions that require a more formal dress or hair do are such things as wedding ceremonies or baptisms.
You will find several choices for formal hair styles: beautiful, romantic and glamorous.
The strategies of the formal event's success would be the detailed planning and also the organization. First, start with the appearance you need to create. Begin with the clothing. Everything should be matched, this is exactly why attempt to choose everything, in the dress towards the add-ons that fit your occasion and than decide which is your decision in the abundance of formal hair styles.
Do your haircut a minumum of one week prior to the formal event to permit your hair to stay lower. Fresh haircuts aren't easy to handle. Then together with your stylist's help have to find the right formal hair styles for you personally. You are able to select a particular hair do from celebs inside a magazine.
Updo hair styles will always be in style. The stylist can modify it to match your personality. Frizzy hair deposited close to the crown with curls framework the face area is extremely feminine. In case your locks are blond and absolutely straight you should use medium length haircut and mild waves.
Layered wavy hair doesn't need any special formal hair styles. Only use some styling foam. Straight hair inside a pony tail is an ideal formal hair do for business conferences.
Any hair do whether it's short or lengthy, curly or straight may become a proper hair do. Short formal hair styles suit the very best on individuals with longer or heart shape faces. Typically the most popular hair styles for brief fur would be the gelled-back look and stylist bob. Lengthy, flowing hair blends completely with all of formal dresses giving more attention and originality towards the face. Lengthy formal hair styles likewise incorporate structured curls, loose waves, loose ringlets or modern updos. Formal updo hair styles, gorgeous and frumpy, would be the greatest formal fashion today that contributes attract the formal dresses and also the occasion too. Double buns, low pony tails, high pony tails and low chignon are couple of from the other formal hair styles for lengthy hair.
This isn't to state that you need to follow these recommendations, but in so doing you instantly complement your natural features, which produces balance and excitement, causing you to more appealing.


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Great for kids or one adult the F-11 is the most phenomenal personal water-craft ever made. In fact, there is absolutely nothing like it on the market today. Although you can take it out on the ocean, this powerhouse of a small boat is ideal for inland lakes and rivers. It's also the perfect starter craft for young boaters and perfect for horse-power or speed restricted areas.
The F-11 is much safer than a jet-ski making it "worry-free" for parents. This rugged little boat is built for speed, but with safety as the top priority. Along with being versatile, the F-11 is incredibly easy to store, maintain and transport.
Hull Type: Fiberglass V-Hull, Ocean Capable
Material: Biaxial Knitted Fiberglass +/- 45 Degrees
Length: 11'9"
Width: 4'7"
Weight: 202 lb.
Dead Rise: 20 Degrees
Draft: 4"
Transom: 15"
Hull Warranty: 5 Years
Recommended Power: 10 HP (not included)
Maximum Power: 15 HP (not included)
Marine Grade UV Resistant Gel coat
Electric Bilge Pump
Navigation Lights
Color Coordinated Marine Vinyl Interior,
Matching Heavy Duty Rub Rail
Marine Carpeting
Grab Handle
Steering System and Wheel
Stainless Steel Bow Eye
Stainless Steel Stern Eyes
Offshore Battery Box
Stainless Steel Hardware
2 Persons or 325 lb.
575 lb. (Persons, Motor and Gear)
Recommended Engine
Maximum Engine 15HP
- This boat complies with US Coast Guard safety standards effective on the date of certification


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A MAN was fined after household waste, including an oven and bed frame, was dumped outside a block of flats.
Anthony Dine pleaded guilty to knowingly causing household waste to be deposited from his vehicle without a waste management licence.
The 26-year-old appeared at Fareham Magistrates' Court after someone saw his van dumping the household rubbish in Franklin Road, Gosport.
The court heard that on April 28, a witness saw people moving out of flats on the roads and load items on to a parked Ford Transit van.
Once loaded, the vehicle drove away, only to return later and off-load a whole range of household items, dumping them on land between the two blocks of flats before driving off.
The items fly-tipped included an oven, bed frame, carpet and an ironing board.
Clearing up after fly-tipping incidents has a serious impact on our budgets as it costs the council heavily.Councillor Graham Burgess
The resident who witnessed the incident had managed to get the registration number of the vehicle and reported it.
With the registration number, officers at the Gosport Borough Council managed to track down the owner of the vehicle and Dine was requested to attend for interview under caution.
During sentencing, the magistrates ordered Dine, of Colesbourne Road, Paulsgrove, to pay Gosport Borough Council £100 compensation/clean-up costs.
He was also ordered to pay £921.21 legal costs.
Councillor Graham Burgess, chairman of the community board at the council said: 'We are delighted to have been successful in this matter and we thank the witness for their help in this matter.
'Clearing up after fly-tipping incidents has a serious impact on our budgets as it costs the council heavily.
'That's why the help of the public in reporting sightings to us can make such a huge difference in these matters.'
Anyone who sees fly-tipping occurring should report the make, registration and colour of the vehicle, plus any description of persons involved to Streetscene on 0800 019 8598.


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I'm delighted, one seriously happy bunny. Because after years of (soul) searching I've finally found my passion, my life purpose, my raison d'etre and it feels great. I suddenly feel more alive than I ever have before.
I read somewhere that when you discover your life purpose, everything starts to fall into place, you begin to experience happy and serendipitous events and positive messages that you are doing the right thing.
I couldn't have asked for a better reaction to this blog and the path that I have chosen to take. The comments people have made and the feedback I've received have blown me away in ways that I never expected.
I'm also surprised by the changes I see in myself. I love writing this blog, setting myself goals to achieve my dreams and working towards them, as well as hearing from people that what I've written has inspired or helped them.
As a result of this newfound passion, it's little wonder that I now find myself spending every spare second working towards making this whole blog thing work. The problem is that I don't have that many spare seconds.
Where does the time go?
During the week, of my 24 hours a day, I spend six hours of it sleeping, eight hours working (my day job), four hours a day commuting and around two hours a day eating, showering and cooking.
This leaves me with approximately four hours a day to do the following:
- Catch up with family
- Socialise with friends
- Spend time on working on this blog
- Spend time working towards my goals
- Doing exercise
- Relaxing
Whilst I love the changes in my life that finding my passion have brought (which include: excitement, drive, commitment, motivation), what I've recently noticed is the thing that seems to have disappeared as a result, is balance. I currently feel that I am lacking balance in my life and here are a few examples of how that manifests:
With only four hours a day of 'free' time, a large chunk of this is currently being spent on working on my blog in terms of content and marketing. If I want to build a successful blog on personal development then it makes sense to put this time in.
However, what this translates into is that I spend more of my free time online than I do in the 'real' world and I spend more of my free time working rather than relaxing or socialising. This has resulted in feeling more than a little tired and run down.
A lesson about balance
The lesson here for me has been to look at how I spend my time and work towards regaining balance in the areas that need it. I've already started on this by reconnecting with friends I haven't seen for a while and making a concerted effort to contact members of my family for a catch up.
Where I know I need to make even more effort is in minimising the time I spend looking at a computer screen. Often, I waste time online in the name of 'working on my blog' rather than being productive and my plan is to put specific time aside for 'work' and using the left over time to relax and connect with people I love.
What does your day look like when you break it down? Are there things that you are doing too little or too much of? Do you have any tips or suggestions for maintaining balance? If so I would love to hear from you.


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Published on March 6, 2014
Author: sacani
Source: slideshare.net
Reports Molecular Gas Clumps from the Destruction of Icy Bodies in the β Pictoris Debris Disk significance level of 4σ, suggesting that it may influence the innermost dust distribution. ALMA also detected the disk in the 12 CO J = 3-2 transition (Fig. 1B), with a clear velocity gradient along the major axis, illustrated in the position-velocity (PV) diagram (Fig. 2). This shows the characteristic distribution of a broad 1 2 3 4 5 W. R. F. Dent, * M. C. Wyatt, A. Roberge, J.-C. Augereau, S. Casassus, S. belt of orbiting gas, with inner and 1 6 1,7 1 2,8 Corder, J. S. Greaves, I. de Gregorio-Monsalvo, A. Hales, A. P. Jackson, outer radii of 50 and 160 AU, and a A. Meredith Hughes,9 A.-M. Lagrange,4 B. Matthews,10 D. Wilner11 peak around 85 AU. No gas emission is 1 seen inside 50 AU. The CO distribution ALMA Santiago Central Offices, Alonso de Córdova 3107, Vitacura, Casilla 763 0355, Santiago, Chile. 2 is, on average, a factor of 2 brighter to Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK. 3Exoplanets and Stellar Astrophysics Lab, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. 4UJF-Grenoble 1/CNRS-INSU, the southwest, and a similar asymmetry Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), UMR 5274, Grenoble, F-38041, France. was seen in the mid-infrared emission 5 Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile. 6Dept. of Astronomy, (12). Unlike the sub-mm continuum, 7 University of St. Andrews, North Haugh, St. Andrews, UK. European Southern Observatory, Karlthe CO clump is offset by ~5 AU above 8 Schwarzschild Str. 2, 85748, Garching, Germany. School of Earth and Space Exploration, Arizona State the main disk plane (Fig. 1B) and is 9 University, ISTB4, 781 E Terrace Rd., Tempe, AZ 85287–6004, USA. Wesleyan University Department of more closely aligned with the inner Astronomy, Van Vleck Observatory, 96 Foss Hill Drive, Middletown, CT 06459, USA. 10National Research planet b Pic b and a secondary disk Council of Canada, Herzberg Astronomy & Astrophysics Programs, 5701 West Saanich Road, Victoria, BC, seen in scattered light (5, 9). Canada, V9E 2E7, and Department of Physics & Astronomy, University of Victoria, Finnerty Road, Victoria, The CO J = 3-2 emission totals 7.6 BC, V8P 5C2, Canada. 11Smithsonian Astrophysical Observatory, 60 Garden St., MS 42, Cambridge, MA 02138, USA. ± 0.8 10–20 W/m2. Assuming a range of possible excitation temperatures *Corresponding author. E-mail: email@example.com from 20 K [measured from UV absorption lines (13)], to 85 K [the dust equiMany stars are surrounded by disks of dusty debris formed in the collisions of librium temperature (10)], this asteroids, comets and dwarf planets. But is gas also released in such events? corresponds to a CO mass of 1.7 1020 Observations at sub-mm wavelengths of the archetypal debris disk around β kg (0.0023MMoon) within a factor of 2. Pictoris show that 0.3% of a Moon mass of carbon monoxide orbits in its debris belt. Toward the star itself, the total CO The gas distribution is highly asymmetric, with 30% found in a single clump 85 AU column is 2.5(+2.5,–1.2) 1015 cm–2 ; refrom the star, in a plane closely aligned with the orbit of the inner planet, β Pic b. sults from UV absorption line measThis gas clump delineates a region of enhanced collisions, either from a mean urements range between 0.6-2.1 1015 motion resonance with an unseen giant planet, or from the remnants of a collision cm–2 (13), indicating that at least 10% of Mars-mass planets. of the CO along this line-of-sight lies in front of the star. Debris disks are the end product of collisional cascades of km-sized The attenuation through the disk due to dust or CO self-shielding is bodies orbiting stars (including the Sun), and are normally thought to low and, at radii >50 AU, CO is destroyed mostly by UV photons from contain negligible gas. At a distance of 19.44 parsec (1) and age of 20 the ambient interstellar medium (ISM) (14). The CO photodissociation million years (2), β Pictoris is one of the closest, brightest and youngest timescale in the unshielded outer disk will be ~120 yrs (15) - substantialexamples. Its edge-on disk was the first to be imaged in scattered light, ly less than the 600-year orbital period at 85 AU. Unless we are observshowing the distribution of micron-sized dust grains (3). Various subse- ing β Pic at a very unusual time (i.e., ≤100 years after a collision) then quent observations have provided evidence of infalling comets within a the CO must be continuously replenished, with a steady-state production few Astronomical Units (AU) of the star (4), a massive planet at ~10 AU rate of ~1.4 1018 kg/yr. The source of CO is likely the icy debris (5), as well as atomic gas extending out to ~300 AU (6); it is still unclear (grains, comets and planetesimals) in the disk (16). In our own solar how these features are linked. By observing such debris disks at mm system, comets are mostly composed of refractory silicate grains togethwavelengths, it is possible to trace the mm-sized dust and, by inference, er with H2O and CO ices, with a typical CO/H2O ratio of 0.01-0.1 (17). the parent bodies of the collisional cascade, known as planetesimals (7). Although CO sublimates at ~20K - substantially less than the 85 K dust We observed β Pic using the Atacama Large Millime- temperature in the β Pic disk - it can be trapped in H2O ice at temperater/submillimeter Array (ALMA) at a wavelength of 870 μm in both the tures up to ~140 K (18), which could occur in radiative equilibrium as continuum and the J = 3-2 12CO line with a resolution of 12AU (8). The close as 30 AU from β Pic (14). At larger distances, photodesorption or continuum image (Fig. 1A) shows maxima in the surface brightness ~60 collisions can release this CO into the gas phase. Photodesorption (a.k.a. AU either side of the star. At separations from 30-80 AU the continuum UV sputtering) of mm-sized ice grains (19) in a dust clump with 10% of is, on average, 15% brighter to the southwest. These results indicate that the total disk mass would produce CO at a rate that is ~10 times lower the mm grains lie in a broad slightly asymmetric belt nearly co-located than our observations show. The CO linewidth measured directly toward with the disk of sub-micron reflecting dust (9). The total flux of 60 ± 6 the star is ~1 km/s (Fig. 2), suggesting the velocity dispersion is lower mJy corresponds to a dust mass of 4.7 ± 0.5 1023 kg (6.4MMoon), if we than the 6km/s thought necessary for collisions to directly vaporize ice assume a standard dust mass opacity (0.15 m2 kg–1 at 850 μm) and tem- (20). However icy parent bodies being shattered in multiple lower velocperature of 85 K (10). ity collisions may release much of the entrapped CO as gas, leaving the The planet β Pic b was close to maximum SW elongation at the time less volatile H2O ice behind. To sustain the gas production rate with a of the observations, with a projected separation of 8.7 AU (11). Its loca- CO ice release fraction of 0.1, the required mass loss of colliding grains tion is coincident with a dip in the continuum surface brightness at a would be ~1.4 1019 kg/yr, equivalent to the destruction of a large com- / http://www.sciencemag.org/content/early/recent / 6 March 2014 / Page 1 / 10.1126/science.1248726
et every 5 min. If sustained over the lifetime of β Pic, ~50MEarth of icy bodies will have been removed. Continual replenishment of CO may explain another puzzle. In the absence of a braking mechanism many of the atomic species such as Na found around β Pic should be blown out from the central star under the force of radiation pressure (21–23). Carbon is overabundant relative to other metals, by factors of 18 to 400 (21, 22), and has been proposed as the mechanism that allows the ionized gas to remain bound to the star. C+ couples to other ions through Coulomb forces; and since it feels weak radiation pressure from the central star, it tends to brake all the gas. The origin of the unusual carbon overabundance may be explained if CO is being rapidly released in the clump, then dissociated and ionized before being spread throughout the disk. In steady state, the relative C+/CO abundance implies that C+ is being removed on a timescale of 3 103104 yrs; since this is several orbital timescales at 85 AU, the braking gas can be spread throughout the disk. If the gas is on circular Keplerian orbits, each point in the PV diagram corresponds to one of two points in the disk. Figure 3 shows possible deprojections of the data to form the face-on gas distribution (8). A compact clump of CO is found at 85 AU radius which contains ~30% of the flux, along with an extended "tail" of emission. The radial distribution of the mm dust can also be derived (8, 12), and shows excess around this radius in the southwest (Fig. 3C). The mm dust shows an abrupt drop in density around 130 AU radius, coincident with a change in slope in the radial distribution of scattered light. This was interpreted as a transition from a dust-producing planetesimal belt to a region dominated by submicron-sized grains blown out by radiation pressure (9, 24). What is the origin of the CO clumps and corresponding mid-infrared and continuum features? There are two possible interpretations, both requiring planet-mass objects in the outer disk, but with different predictions for the deprojected gas distribution. In the first (Fig. 3A), outward migration of a planet traps planetesimals into both the 2:1 and 3:2 mean motion resonances, resulting in a distribution with two clumps of asymmetric brightness on opposite sides of the star that orbit with the planet (25). Planetesimal collisions would occur most frequently in the clumps which would then be the most vigorous production sites of both CO and the short-lived micron-sized grains seen in mid-infrared images (12). The morphology of the clumps constrains the planet's mass and migration parameters (25). Notably the planet must be >10MEarth to have captured material into its 2:1 resonance, and it would currently be close to the inner edge of the gas/dust belt, ~90 degrees in front of the SW clump. The CO clump's "tail" would point in the opposite direction to the rotation, and its' length given by the ratio of CO photodissociation lifetime to the synodic period. The alternative interpretation (Fig. 3B) is that the CO and micronsized dust originate in a single recent collision (12, 26). Since the clump also contributes ~10% of the flux in our sub-mm continuum image, the parent body must have ~Mars mass, as giant impacts typically release ~10% of the progenitor's mass as debris (27). While collisional debris persists in a clump for ~100 yr after such an event, it is more likely that the collision occurred ~0.5 Myr ago, with the asymmetry arising because the orbits of all collisional debris pass through the collision point, a region which would retain a high density and collision rate (26). Such a clump would be stationary, and the CO "tail" would lie in the rotation direction, with a length given by the ratio of photodissociation time to sidereal period (Fig. 3B). Tentative evidence has been published for the clump's motion (28), which if confirmed would favor the resonance interpretation. Either way these observations provide a valuable opportunity to ascertain the prevalence of planet-sized objects at large orbital distances in this disk. The CO gas detected in β Pic is unusual among debris disks. So far, two others have been detected in CO [49 Cet and HD21997 (16)] and one in OI [HD172555 (29)]. Most debris disks are presumed to contain icy grains, so we would expect all such systems to host CO and its photodissociation products. The high collision rates found in clumps may substantially enhance the gas abundance. If CO is formed in collisions, its brightness will scale as the collision rate, which is proportional to vr nd2, where vr is the collision velocity and nd is the number of dust grains. Both nd and vr are enhanced in clumps due to resonances and giant impacts, increasing collision rates by factors of up to 10-100 (7, 26). The presence of these clumps can increase the overall collision rate and CO flux from a disk by an order of magnitude. The CO and compact clump in the β Pic disk indicates a period of intense activity, driven by planets or planet collisions. References and Notes 1. F. van Leeuwen, Validation of the new Hipparcos reduction. Astron. Astrophys. 474, 653–664 (2007). doi:10.1051/0004-6361:20078357 2. A. S. Binks, R. D. Jeffries, A lithium depletion boundary age of 21 Myr for the beta Pictoris moving group. Mon. Not. R. Astron. Soc. 438, L11–L15 (2014). doi:10.1093/mnrasl/slt141 3. B. A. Smith, R. J. Terrile, A circumstellar disk around β Pictoris. Science 226, 1421–1424 (1984). doi:10.1126/science.226.4681.1421 4. A. Vidal-Madjar et al., Astron. Astrophys. 290, 245 (1994). 5. A.-M. Lagrange, M. Bonnefoy, G. Chauvin, D. Apai, D. Ehrenreich, A. Boccaletti, D. Gratadour, D. Rouan, D. Mouillet, S. Lacour, M. Kasper, A giant planet imaged in the disk of the young star Pictoris. Science 329, L57 (2010). doi:10.1126/science.1187187 6. A. Brandeker, R. Liseau, G. Olofsson, M. Fridlund, The spatial structure of the β Pictoris gas disk. Astron. Astrophys. 413, 681–691 (2004). doi:10.1051/0004-6361:20034326 7. M. C. Wyatt, Dust in resonant extrasolar Kuiper belts: Grain size and wavelength dependence of disk structure. Astrophys. J. 639, 1153–1165 (2006). doi:10.1086/499487 8. Materials and methods are available as supplementary materials on Science Online. 9. D. A. Golimowski, D. R. Ardila, J. E. Krist, M. Clampin, H. C. Ford, G. D. Illingworth, F. Bartko, N. Benítez, J. P. Blakeslee, R. J. Bouwens, L. D. Bradley, T. J. Broadhurst, R. A. Brown, C. J. Burrows, E. S. Cheng, N. J. G. Cross, R. Demarco, P. D. Feldman, M. Franx, T. Goto, C. Gronwall, G. F. Hartig, B. P. Holden, N. L. Homeier, L. Infante, M. J. Jee, R. A. Kimble, M. P. Lesser, A. R. Martel, S. Mei, F. Menanteau, G. R. Meurer, G. K. Miley, V. Motta, M. Postman, P. Rosati, M. Sirianni, W. B. Sparks, H. D. Tran, Z. I. Tsvetanov, R. L. White, W. Zheng, A. W. Zirm, Hubble Space Telescope ACS multiband coronagraphic imaging of the debris disk around β Pictoris. Astron. J. 131, 3109–3130 (2006). doi:10.1086/503801 10. W. R. F. Dent, H. J. Walker, W. S. Holland, J. S. Greaves, Models of the dust structures around Vega-excess stars. Mon. Not. R. Astron. Soc. 314, 702–712 (2000). doi:10.1046/j.1365-8711.2000.03331.x 11. G. Chauvin, A.-M. Lagrange, H. Beust, M. Bonnefoy, A. Boccaletti, D. Apai, F. Allard, D. Ehrenreich, J. H. V. Girard, D. Mouillet, D. Rouan, Orbital characterization of the β Pictoris b giant planet. Astron. Astrophys. 542, A41 (2012). doi:10.1051/0004-6361/201118346 12. C. M. Telesco, R. S. Fisher, M. C. Wyatt, S. F. Dermott, T. J. Kehoe, S. Novotny, N. Mariñas, J. T. Radomski, C. Packham, J. De Buizer, T. L. Hayward, Mid-infrared images of β Pictoris and the possible role of planetesimal collisions in the central disk. Nature 433, 133–136 (2005). Medline doi:10.1038/nature03255 13. A. Roberge, P. D. Feldman, A. M. Lagrange, A. Vidal-Madjar, R. Ferlet, A. Jolly, J. L. Lemaire, F. Rostas, High‐resolution Hubble Space Telescope STIS spectra of C I and CO in the β Pictoris circumstellar disk. Astrophys. J. 538, 904–910 (2000). doi:10.1086/309157 14. I. Kamp, F. Bertoldi, Astron. Astrpophys. 353, 276 (2001). 15. R. Visser, E. F. van Dishoeck, J. H. Black, The photodissociation and chemistry of CO isotopologues: Applications to interstellar clouds and circumstellar disks. Astron. Astrophys. 503, 323–343 (2009). doi:10.1051/0004-6361/200912129 16. B. Zuckerman, I. Song, A 40 Myr old gaseous circumstellar disk at 49 Ceti: Massive CO-rich comet clouds at young A-type stars. Astrophys. J. 758, 77 (2012). doi:10.1088/0004-637X/758/2/77 17. K. I. Oberg, A. C. A. Boogert, K. M. Pontoppidan, S. van den Broek, E. F. / http://www.sciencemag.org/content/early/recent / 6 March 2014 / Page 2 / 10.1126/science.1248726
van Dishoeck, S. Bottinelli, G. A. Blake, N. J. Evans, The Spitzer ice legacy: Ice evolution from cores to protostars. Astrophys. J. 740, 109 (2011). doi:10.1088/0004-637X/740/2/109 18. M. P. Collings, J. W. Dever, H. J. Fraser, M. R. S. McCoustra, D. A. Williams, Carbon monoxide entrapment in interstellar ice analogs. Astrophys. J. 583, 1058–1062 (2003). doi:10.1086/345389 19. A. Grigorieva, Ph. Thebault, P. Artymowicz, A. Brandeker, Survival of icy grains in debris discs. Astron. Astrophys. 475, 755–764 (2007). doi:10.1051/0004-6361:20077686 20. A. G. G. M. Tielens, C. F. McKee, C. G. Seab, D. J. Hollenbach, The physics of grain-grain collisions and gas-grain sputtering in interstellar shocks. Astrophys. J. 431, 321 (1994). doi:10.1086/174488 21. A. Roberge, P. D. Feldman, A. J. Weinberger, M. Deleuil, J.-C. Bouret, Stabilization of the disk around β Pictoris by extremely carbon-rich gas. Nature 441, 724 (2006). doi:10.1038/nature04832 22. J.-W. Xie, A. Brandeker, Y. Wu, On the unusual gas composition in the β Pictoris debris disk. Astrophys. J. 762, 114 (2013). doi:10.1088/0004637X/762/2/114 23. R. Fernandez, A. Brandeker, Y. Wu, Braking the gas in the β Pictoris disk. Astrophys. J. 643, 509–522 (2006). doi:10.1086/500788 24. J. C. Augereau, R. P. Nelson, A. M. Lagrange, J. C. B. Papaloizou, D. Mouillet, Dynamical modeling of large scale asymmetries in the β Pictoris dust disk. Astron. Astrophys. 370, 447–455 (2001). doi:10.1051/00046361:20010199 25. M. C. Wyatt, Resonant trapping of planetesimals by planet migration: Debris disk clumps and Vega's similarity to the solar system. Astrophys. J. 598, 1321–1340 (2003). doi:10.1086/379064 26. A. P. Jackson, M. C. Wyatt, Debris from terrestrial planet formation: The Moon-forming collision. Mon. Not. R. Astron. Soc. 425, 657–679 (2012). doi:10.1111/j.1365-2966.2012.21546.x 27. S. T. Stewart, Z. M. Leinhardt, Collisions between gravity-dominated bodies. II. The diversity of impact outcomes during the end stage of planet formation. Astrophys. J. 751, 32 (2012). doi:10.1088/0004-637X/751/1/32 28. D. Li, C. M. Telesco, C. M. Wright, The mineralogy and structure of the inner debris disk of β Pictoris. Astrophys. J. 759, L81 (2012). doi:10.1088/0004637X/759/2/81 29. P. Riviere-Marichalar, D. Barrado, J.-C. Augereau, W. F. Thi, A. Roberge, C. Eiroa, B. Montesinos, G. Meeus, C. Howard, G. Sandell, G. Duchêne, W. R. F. Dent, J. Lebreton, I. Mendigutía, N. Huélamo, F. Ménard, C. Pinte, HD 172555: Detection of 63 μm [OI] emission in a debris disc. Astron. Astrophys. 546, L8 (2012). doi:10.1051/0004-6361/201219745 Acknowledgments: This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00087.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. Partial financial support for SC, MCW and AH was provided by Millenium Nucleus P10-022-F (Chilean Ministry of Economy). AR acknowledges support by the Goddard Center for Astrobiology, part of the NASA Astrobiology Institute. MCW was supported by the European Union through ERC grant number 279973, IdG acknowledges support from MICINN (Spain) AYA2011-30228-C03 grant (including FEDER funds), APJ was supported by an STFC postgraduate studentship, and JCA acknowledges the French National Research Agency (ANR) for support through contract ANR-2010 BLAN-0505-01 (EXOZODI). Supplementary Materials www.sciencemag.org/cgi/content/full/science.1248726/DC1 Materials and Methods References 19 November 2013; accepted 20 February 2014 Published online 6 March 2014 10.1126/science.1248726 / http://www.sciencemag.org/content/early/recent / 6 March 2014 / Page 3 / 10.1126/science.1248726
Fig. 1. Images of β Pic using ALMA in continuum and line emission. Both have been rotated by +29 degrees, the position angle of the main dust disk. The beam size (0.56 0.71 arcsec) is shown lower left, and the locations of the star and planet on the date of observations are indicated by the asterisk and the cross. (A) Continuum emission at 870 μm from the mm dust; the rms noise –1 level is 61 μJy beam . (B) Total J = 3-2 CO line emission (rest frequency –20 –2 345.796 GHz); the noise level is 0.02 10 W m . The planes of the main and secondary dust disks (9) are shown by the dashed lines. / http://www.sciencemag.org/content/early/recent / 6 March 2014 / Page 4 / 10.1126/science.1248726
Fig. 2. Velocity distribution along disk major axis. This shows the observed velocity of the CO emission relative to the velocity measured toward the star (which has a centroid of +20.3 ± 0.1 km/s, in the barycentric reference frame). Gas on the brighter SW side is approaching us; the two dashed white lines represent the velocity we would measure from gas at the inner and outer radii of the CO belt. The solid red lines show the true orbital velocity, the maximum observed velocity from gas at the tangential point, as a function of distance from the star, assuming a stellar mass of 1.75Msolar. Contours are 10, 20, 30, 40, 60, 80% of the peak (0.06 Jy/beam). The spectral/spatial resolution is illustrated lower left. / http://www.sciencemag.org/content/early/recent / 6 March 2014 / Page 5 / 10.1126/science.1248726
Fig. 3. Deprojected distributions of gas and dust around β Pic (8). (A and B) Two possible face-on distributions of the CO assuming circular orbital motion. (A) The twoclump distribution, interpreted as mean-motion resonances with an inner planet. In this case the bright southwest resonance lies on the far side of the star and is approaching us. (B) Single clump distribution, interpreted as a collision of ~Mars-mass objects; in this case the southwest clump is stationary and the "tail" of CO points in the direction of rotation. (C) Radial distribution of mm-sized dust in the southwest and northeast sectors of the disk, obtained by fitting consecutive annuli to the continuum distribution on the two sides (12). The dashed line is an axisymmetric model for the parent body distribution predicted from scattered light images of the sub-micron grains (24). Surface 2 2 density units are cross-section area per unit disk area, in AU /AU . / http://www.sciencemag.org/content/early/recent / 6 March 2014 / Page 6 / 10.1126/science.1248726


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#HIMYM, Season 9 Episode 22
Episode 22 "The End of the Aisle" aired on Monday March 24.
The wedding is here, Robin & Barney's wedding day is upon us and there is some serially doubting going on, cold feet anyone?
We get to find out that Ted actually swam to fish out the locket after "crazy" through it in the river and when Robin says that she doesn't understand why she is marrying Barney when he couldn't find the locket for her, Ted gives it to Barney and says that he has to give it to Robin and say that he found it.
Robin meets the mother when she is trying to run out of the church and the mother tells Robin to close her eyes and take three deep breaths because "three deep breaths can change everything"
The episodes ends with Barney and Robin finally making it down the aisle and next week is the 2 hour finale episode!
What can we expect when Ted finally meets the mother? Are we getting her name or will she forever be "the mother"?
Just a side note, I absolutely love Cristin Milioti as the mother, she is just fantastic ♥


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Book #28: Founding Brothers: The Revolutionary Generation, Joseph J. Ellis
The Revolutionary era was an important and iconic era of our history. And with 200 years of retrospection, it is often easy to romanticize the constitutional era and believe that it was a period of ideological clarity and political unanimity. We often view the founding fathers as a generation of compatriots who worked together to build the nation we enjoy today. And while these men were all motivated by a unified vision for an American nation, their ideas for how that nation should be build were often vastly different. This is a fascinating look into the politics of the 1790's and is a detailed accounting of a generation who gave of their lives, fortunes and sacred honor to give us the nation that we enjoy today.
#2016bookreview #mattreadinglist


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Dutch smokers win partial reprieve
Interesting news from the Netherlands where reports suggest that the ban on smoking will be lifted in small bars that are run and therefore staffed by one-man businesses. According to Radio Netherlands:
Owners of small pubs in the Netherlands have welcomed the lifting of a smoking ban imposed on the hospitality industry in 2008. The partial scrapping of the measure was announced on Tuesday.
The incoming right-wing government is responding to persistent complaints from one-man businesses who argued that the smoking ban was meant to guarantee staff a smoke-free working environment. Since they had no employees, their small pubs didn't need the smoking ban, the owners claimed. The ban will remain in force, however, for pubs, restaurants and the like which are run with personnel.
Secretary Wiel Maessen of the 1250 small pubs' umbrella group KHO said "I lit an extra cigarette when I heard the news." He added that despite his satisfaction on behalf of his members, the fight would not be over until the ban was lifted for the entire sector.
Ton Wurtz, who runs the Dutch smokers' group Stichting Rokersbelangen and has been working with Wiel Maessen, adds a word of caution, however, pointing out in an email to me that the political situation in the Netherlands remains unsettled and the country could face a new election very soon.
Nevertheless it shows what can be achieved if everyone works together. See Smoking ban on trial in The Hague and Demonstrators gather in The Hague.
In February 2006, a few days after MPs voted for a smoking ban in England, Ton and his colleague Dick Engel attended the Forest Awards at the Groucho Club in Soho.
According to our press release:
Forest's 'International Award' went to Dick Engel and Ton Wurtz of the Dutch smokers' lobby group Stichting Rokersbelangen who flew in from Amsterdam to accept their prize.
Other award winners that year included David Hockney, inventor Trevor Baylis, Philip Davies MP, the Institute of Ideas' Claire Fox, artist Maggi Hambling, and the then Health Secretary Patricia Hewitt:
In the face of fierce competition, said Forest, 'Killjoy of the Year' was won by Health Secretary Patricia Hewitt. "Thanks to Nanny Hewitt," said director Simon Clark, "not only will it be a crime to smoke in any indoor public place, but if we wanted to set up a private club run by smokers for smokers, that would illegal too! So much for civil liberties."
Jeremy Clarkson, it may interest you to know, was declared 'Rat of the Year' "for supporting a ban on smoking in all public places because it will allegedly help him give up". The award, Forest announced, had been made with some regret because Clarkson had previously been something of a hero. "Unfortunately, the rat has left the sinking ship."


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Tasers drawn on '400 children in 2013'
MORE than 400 children have had tasers drawn on them by police in England and Wales in 2013, figures obtained by the BBC show.
The Home Office Taser database, seen by BBC Radio 5 live, shows a 38% increase on 2012 in the number of children who had a taser aimed at them. Tasers were fired 37 times at 10 to 17-year-olds.
Ex-Home Secretary David Blunkett, who introduced Tasers, called for a review.
The Home Office said Theresa May has asked for a review of Taser usage.
The figures obtained through a Freedom of Information request show the youngest person to have a Taser aimed at them was 11, while the youngest person fired on was 14.
The oldest person to have one pointed at them was 85 and the oldest person actually fired on was 82.
The Home Office has not released Taser statistics broken down by age before, and warns that they are not wholly reliable because the age figures may be police estimates.
Tasers fire dart-like electrodes into a person's body and are used to incapacitate suspects.Speaking to 5 live, Mr Blunkett called for chief constables and police and crime commissioners in England and Wales to look at who was authorised to use Tasers and whether there were alternatives.
"I think it's time for a review that incorporates the use of Tasers with advice and support on how to deal with difficult situations," he said.
"For a youngster, 11 years old, a Taser is not in my view an appropriate way of dealing with a situation which clearly must have been out of hand, but where we need to train people to use much more traditional alternatives."The Association of Chief Police Officers (Acpo) says under-18s are involved in a lot of violent crime, and that any use has to be justifiable in court.
Commander Neil Basu said he did not want to comment on individual cases but it was important to understand the circumstances surrounding the use of a Taser.
"We have to remember that children can commit violent crime too. The police are paid to intervene in those situations and Taser can be an appropriate use of force," he said.
"If that 14-year-old is committing a violent act towards a member of the public or to an officer, or if they are self-harming, then our job is to make sure that that stops in the safest way possible.
"And in certain circumstances, Taser is that option."Daniel Dove was 22 when he was tasered in a police cell in Trowbridge, Wiltshire.
He says it was for flicking his underpants at a police officer during a strip search.
He had been arrested for being drunk and disorderly and assault, but the case was later dropped.
"I'd say it's like being shocked by a cattle fence, but 50,000 times stronger," he said.
"I felt like I was paralysed… I couldn't move my hand or my body.
"It wasn't a very nice experience to have."
The officer involved was later charged with assault and misconduct, but cleared by a jury at Bristol Crown Court.
Iain Gould, a solicitor at DPP Law, who has been involved in a number of cases involving claims of inappropriate use of Tasers, said his concern was "mission creep" as they become more commonly used.
"Several years ago, Tasers were deployed to certain trained firearms officers," he said.
"We now have a situation where routine rank-and-file officers are being given Tasers to use.
"My concern is that it has got out of hand and what we are seeing is effectively militarisation by stealth."That is not a description Commander Neil Basu said he recognised.
"I disagree with that entirely, but I do know it is a concern," he said.
"This is a very emotional subject but police forces, police officers using force, that is one of our absolute key responsibilities that the public have chosen to give us.
"And if we choose to abuse that then we would lose the power.
"There are no people more accountable than firearms and Taser-trained officers. So if an officer uses that power inappropriately, absolutely they should be held accountable to the law."According to Home Office guidance, only authorised firearms officers and specially trained units can use Tasers.
Officers trained in the use of Tasers must consider the vulnerability of the individual and factors such as age and stature form part of this assessment.
A Home Office spokesman said: "The home secretary has been clear that the use of sensitive police powers, such as stop and search, mental health and the use of force, warrant proper accountability and transparency to ensure that they are being used appropriately."Taser is an important tactical option to help specially trained police officers resolve potentially violent situations safely, but it is right that its use is subject to the same level of scrutiny."
He said a review by Chief Constable David Shaw would look at how Taser is being used, who it is being used on and what the outcomes are."
In January, the Police Federation voted for all front-line police in England and Wales to be offered Tasers in light of the increased terrorism threat.
Head of the federation, Steve White, said the devices would help protect against "dangerous people" who could be preparing to attack officers.
However some critics, including Christopher Salmon, a Welsh police and crime commissioner, said the move would be a mistake.
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Dating in Casper is not exactly a walk in the park.
"Jen and Casper spend all their free time with each other. "They work together as well, so time together is plentiful.
They like being with each other and find a lot of time to hang out with each other." The superstar and her former backup dancer, who split in June 2014 after two years of dating, first had us guessing about their relationship status when they were caught kissing on the set of on March 26.
"They have a wonderful working relationship and a wonderful real relationship!
Plus, her kids love him." So it totally makes sense why the duo have been connected at the hip lately!
But as expected from someone who reaches millions of people every day, he doesn't share about his personal life.
As of now, Caspar is single, but quite a few ladies have stepped in and out of the You Tuber's life. Others, however, are merely speculation and rumors.
She and former-beau Casper Smart, 28, have been hanging out more than ever as of late — and many fans are speculating that the two have begun to reestablish their relationship. Lo and Casper are having difficulties spending time apart from each other!
"Jennifer and Casper just get each other," a source tells Hollywood EXCLUSIVELY.
: "I'm single right now, thank you." Hmm, are you sure about that Jenny?Tags: Adult Dating, affair dating, sex dating


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I just got back from a short trip which was a much needed break from our busy lives. Though I wish it could last longer, I shall be thankful that this trip happened! I have never packed so light before in my life. Had no choice this time cause I did not check-in any baggage. Surprisingly, the amount of clothes I packed was just nice for a four day trip! Noticed I tend to pack neutrals during trips to make outfits easier to match. Anyway, I cannot wait to show you the pictures but before that here's a couple of outfit photos from last week.
|Wearing my new Supre dress with my comfiest shoes and cardi, and of course my favourite H&M necklace!