'Copernicus' observations of extragalactic X-ray sources

Details 'Copernicus' observations of extragalactic X-ray sources 'Copernicus' observations of extragalactic X-ray sources

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..42..249f&link_type=abstract

(COSPAR, Symposium on Fast Transients in X- and Gamma-Rays, Varna, Bulgaria, May 29-31, 1975.) Astrophysics and Space Science, v

Astronomy and Astrophysics

Astronomy

1

Extraterrestrial Radiation, Oao 3, Satellite Observation, Spaceborne Astronomy, X Ray Sources, Black Holes (Astronomy), Curve Fitting, Magellanic Clouds, Neutron Stars, Quasars, Radiant Flux Density, Supernova Remnants

Scientific paper

The MSSL X-ray detectors on Copernicus have been used to study a number
of extragalactic objects. At least three classes of unresolved sources
are found and we suggest that accretion may be the dominant mechanism.
The mass of the accreting object then determines the X-ray emission
properties.

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