The Physical and Chemical Properties of Circumstellar       Matter
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Evolved stars of masses similar or slightly greater than that of                the sun evolve through the so-called red giant region.  They are                cool, luminous stars, and they lose mass via strong stellar                     winds.  The winds form circumstellar shells of gas and dust,                    known as planetary nebulae.  The Principal Investigator proposes                to study this kind of mass loss and the formation of planetary                  nebulae.  Both observations and theory will be part of this work.               The emphasis will be on the physics and chemistry of the mass                   loss process.
{'FirstName': 'Patrick', 'LastName': 'Huggins', 'PI_MID_INIT': 'J', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Patrick J Huggins', 'EmailAddress': 'patrick.huggins@nyu.edu', 'PI_PHON': '2129987717', 'NSF_ID': '000191263', 'StartDate': '03/15/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'New York University', 'CityName': 'NEW YORK', 'ZipCode': '100121019', 'PhoneNumber': '2129982121', 'StreetAddress': '70 WASHINGTON SQ S', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'New York', 'StateCode': 'NY', 'CONGRESSDISTRICT': '10', 'CONGRESS_DISTRICT_ORG': 'NY10', 'ORG_UEI_NUM': 'NX9PXMKW5KW8', 'ORG_LGL_BUS_NAME': 'NEW YORK UNIVERSITY', 'ORG_PRNT_UEI_NUM': 'NX9PXMKW5KW8'}
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{'Code': '1215', 'Text': 'STELLAR ASTRONOMY & ASTROPHYSC'}
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