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X-ray astronomy from Uhuru to HEAO-1

Journal Article · · J. Wash. Acad. Sci.; (United States)
OSTI ID:6512376
The nature of galactic and extragalactic X-ray sources is investigated using observations made with nine satellites and several rockets. The question of X-ray pulsars being neutron stars or white dwarfs is considered, as is the nature of Population II and low-luminosity X-ray stars, the diffuse X-ray emission from clusters of galaxies, the unidentified high-galactic-latitude (UHGL) sources, and the unresolved soft X-ray background. The types of sources examined include binary pulsars, Population II X-ray stars (both nonbursters and bursters) inside and outside globular clusters, coronal X-ray emitters, and active galactic nuclei. It is concluded that: (1) X-ray pulsars are strongly magnetized neutron stars formed in the evolution of massive close binaries, (2) all Population II X-ray stars are weakly magnetized or nonmagnetic neutron stars accreting from low-mass companions in close binary systems, (3) the diffuse emission from clusters is thermal bremsstrahlung of hot matter processed in stars and swept out by ram pressure exerted by the intergalactic gas, (4) most or all of the UHGL sources are active galactic nuclei, and (5) the soft X-ray background is emission from a hot component of the interstellar medium.
Research Organization:
MIT, Cambridge, MA
OSTI ID:
6512376
Journal Information:
J. Wash. Acad. Sci.; (United States), Journal Name: J. Wash. Acad. Sci.; (United States) Vol. 71; ISSN JWASA
Country of Publication:
United States
Language:
English