Studies in Stellar Structure and Evolution
{'Code': '03020400', 'Directorate': {'Abbreviation': 'MPS', 'LongName': 'Direct For Mathematical & Physical Scien'}, 'Division': {'Abbreviation': 'AST', 'LongName': 'Division Of Astronomical Sciences'}}
{'SignBlockName': 'Edward G. Schmidt', 'PO_EMAI': None, 'PO_PHON': None}
The study of the evolution of stars is important because it deals               with such topics as the synthesis of the elements (including                    those needed for the making of planets and life), the age of the                galaxy and the universe, and the evolution of galaxies (including               the evolution of our own galaxy, the Milky Way).  For millions or               billions of years, stars typically evolve rather quiescently.                   However, occasionally their evolution is punctuated by explosions               (e.g., supernovae), internal upheavels (e.g., shell flashes), or                mergers of two nearby stars.  This proposal addresses these                     episodic events by computer modelling of stars in the mass range                like our sun and stars that are 8 to 12 times as massive.
{'FirstName': 'Icko', 'LastName': 'Iben', 'PI_MID_INIT': None, 'PI_SUFX_NAME': 'Jr.', 'PI_FULL_NAME': 'Icko Iben', 'EmailAddress': None, 'PI_PHON': None, 'NSF_ID': '000305952', 'StartDate': '11/01/1988', '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}
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{'Code': '1215', 'Text': 'STELLAR ASTRONOMY & ASTROPHYSC'}
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