Physical Parameters of White Dwarfs and Links to Previous   Evolution
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
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White dwarfs constitute the most common end stage in stellar                    evolution.  The Principal Investigator proposes to investigate                  the chemical abundance and the structure of white dwarfs (in                    particular those with hydrogen-dominated atmospheres), to                       determine their masses, rotation rates, and magnetic fields, and                to search for white dwarfs in young galactic clusters in order                  to place constraints on the kinds of young stars that give rise                 to white dwarfs.  The ultimate goal of the proposed work is to                  obtain information about the physical processes that operate                    during the course of stellar evolution that leads up to white                   dwarfs.
{'FirstName': 'Detlev', 'LastName': 'Koester', 'PI_MID_INIT': None, 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Detlev Koester', 'EmailAddress': None, 'NSF_ID': '000357760', 'StartDate': '01/01/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'Louisiana State University', 'CityName': 'BATON ROUGE', 'ZipCode': '708030001', 'PhoneNumber': '2255782760', 'StreetAddress': '202 HIMES HALL', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'Louisiana', 'StateCode': 'LA', 'CONGRESSDISTRICT': '06', 'CONGRESS_DISTRICT_ORG': 'LA06', 'ORG_UEI_NUM': 'ECQEYCHRNKJ4', 'ORG_LGL_BUS_NAME': 'LOUISIANA STATE UNIVERSITY', 'ORG_PRNT_UEI_NUM': 'Z7ZNZH7LJ778'}
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{'Code': '1215', 'Text': 'STELLAR ASTRONOMY & ASTROPHYSC'}
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