High Precision Radial Velocity Study of Young Stars
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
{'SignBlockName': 'minette wilson', 'PO_EMAI': None, 'PO_PHON': None}
Stars form in interstellar clouds of gas and dust that are                      extremely cool, clumpy, and in a general state of turbulence.                   This turbulence is passed on to newly formed stars in the form of               stellar motions.  The Principal Investigator proposes to study                  the motions of newly formed stars in star forming regions, using                as a data base roughly 800 high-precision radial velocity                       measurements of some 300 low-mass pre-main sequence stars.  The                 aim of the investigation is to determine the initial conditions                 and early evolution of stars.
{'FirstName': 'Robert', 'LastName': 'Mathieu', 'PI_MID_INIT': 'D', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Robert D Mathieu', 'EmailAddress': 'mathieu@astro.wisc.edu', 'NSF_ID': '000237740', 'StartDate': '01/01/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'University of Wisconsin-Madison', 'CityName': 'MADISON', 'ZipCode': '537151218', 'PhoneNumber': '6082623822', 'StreetAddress': '21 N PARK ST STE 6301', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'Wisconsin', 'StateCode': 'WI', 'CONGRESSDISTRICT': '02', 'CONGRESS_DISTRICT_ORG': 'WI02', 'ORG_UEI_NUM': 'LCLSJAGTNZQ7', 'ORG_LGL_BUS_NAME': 'UNIVERSITY OF WISCONSIN SYSTEM', 'ORG_PRNT_UEI_NUM': None}
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{'Code': '121500', 'Text': 'STELLAR ASTRONOMY & ASTROPHYSC'}
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