High Resolution Observational Studies of the Structure and  Evolution of Galaxies
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
{'SignBlockName': 'Millissa J. Evans', 'PO_EMAI': None, 'PO_PHON': None}
The research is aimed at determining the distribution, motions                  and physical conditions of the various components of the                        interstellar medium in galaxies.  The purpose is to study the                   relationship of these components to each other, to the spiral                   structure, and to the star formation processes in galaxies.                     While the general evolutionary cycle between the interstellar                   medium and the stars in galaxies is understood, the detailed                    underlying processes are still not clearly delineated.                                                                                                          In order to study the interstellar medium in external galaxies                  with sufficient resolution, the Principal Investigators will use                the relatively new Hat Creek millimeter-wavelength telescope to                 observe the neutral atomic hydrogen (HI) component and the Very                 Large Array (VLA) radio telescope to observe the molecular                      component and the relativistic electrons.  An optical imaging                   Fabry-Perot spectrometer will be used to probe the ionized gas.                                                                                                 Such comparative detailed analyses will further the understanding               of the basic processes of galactic evolution.  How galaxies                     evolve with time has relevance to many basic questions in                       astronomy such as galaxy formation, cosmology, and the origin of                the structure of galaxies and of their morphological types.
[{'FirstName': 'Ronald', 'LastName': 'Allen', 'PI_MID_INIT': 'J', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Ronald J Allen', 'EmailAddress': 'rjallen@stsci.edu', 'PI_PHON': '4103384574', 'NSF_ID': '000100566', 'StartDate': '05/01/1988', 'EndDate': None, 'RoleCode': 'Co-Principal Investigator'}, {'FirstName': 'K. Y.', 'LastName': 'Lo', 'PI_MID_INIT': None, 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'K. Y. Lo', 'EmailAddress': 'flo@nrao.edu', 'PI_PHON': '4342960221', 'NSF_ID': '000090597', 'StartDate': '05/01/1988', 'EndDate': None, 'RoleCode': 'Principal Investigator'}]
{'Name': 'University of Illinois at Urbana-Champaign', 'CityName': 'URBANA', 'ZipCode': '618013620', 'PhoneNumber': '2173332187', 'StreetAddress': '506 S WRIGHT ST', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'Illinois', 'StateCode': 'IL', 'CONGRESSDISTRICT': '13', 'CONGRESS_DISTRICT_ORG': 'IL13', 'ORG_UEI_NUM': 'Y8CWNJRCNN91', 'ORG_LGL_BUS_NAME': 'UNIVERSITY OF ILLINOIS', 'ORG_PRNT_UEI_NUM': None}
{'Name': None, 'CityName': None, 'StateCode': None, 'ZipCode': None, 'StreetAddress': None, 'CountryCode': None, 'CountryName': None, 'StateName': None, 'CountryFlag': None, 'CONGRESSDISTRICT': None, 'CONGRESS_DISTRICT_PERF': '""'}
{'Code': '1217', 'Text': 'EXTRAGALACTIC ASTRON & COSMOLO'}
{'url': 'https://www.nsf.gov/awardsearch/download?DownloadFileName=1987&All=true', 'xml': '8715905.xml'}