On the nature of the galactic bulge X-ray sources

Details On the nature of the galactic bulge X-ray sources On the nature of the galactic bulge X-ray sources

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....67l..25m&link_type=abstract

Astronomy and Astrophysics, vol. 67, no. 3, July 1978, p. L25-L28.

Astronomy and Astrophysics

Astronomy

88

Binary Stars, Galactic Bulge, X Ray Astronomy, X Ray Stars, Angular Distribution, Late Stars, Radiation Distribution, Stellar Luminosity, Stellar Models

Scientific paper

Binary configurations containing a low mass primary, with a compact object having a negligible magnetic field are assumed to provide the basis for a model in which the main observable properties of galactic X-ray sources are as follows: no X-ray pulsations, rare incidence of eclipse, soft X-ray spectrum, and a lowered ratio of optical to X-ray luminosity. Sco X-1 and Cyg X-2 are studied together with galactic-bulge and globular-cluster sources to provide empirical support for the model.

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