Determining the Physical Properties of the Low-Mass X-ray   Binaries
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{'SignBlockName': 'Edward G. Schmidt', 'PO_EMAI': None, 'PO_PHON': None}
Low mass X-ray binaraies (LMXBs) are stellar binary systems                     consisting of a low-mass mass-losing star and a neutron star or,                in some cases, a black hole.  The neutron star or black hole                    accrete matter lost by the companion star.  The accretion                       generally occurs via a disk and includes X-ray emission,                        flickering, and outbursts.  The Principal Investigator proposes                 to study LMXBs in our galaxy and in the Large Magellanic Cloud                  and to determine mass transfer rates, the masses and radii of                   the component stars, and the range of diversity of these very                   interesting systems.
{'FirstName': 'Anne', 'LastName': 'Cowley', 'PI_MID_INIT': 'P', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'Anne P Cowley', 'EmailAddress': 'anne.cowley@asu.edu', 'NSF_ID': '000108207', 'StartDate': '01/01/1989', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'Arizona State University', 'CityName': 'TEMPE', 'ZipCode': '852813670', 'PhoneNumber': '4809655479', 'StreetAddress': '660 S MILL AVENUE STE 204', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'Arizona', 'StateCode': 'AZ', 'CONGRESSDISTRICT': '04', 'CONGRESS_DISTRICT_ORG': 'AZ04', 'ORG_UEI_NUM': 'NTLHJXM55KZ6', 'ORG_LGL_BUS_NAME': 'ARIZONA STATE UNIVERSITY', 'ORG_PRNT_UEI_NUM': None}
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{'Code': '1215', 'Text': 'STELLAR ASTRONOMY & ASTROPHYSC'}
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