Infrared studies of X-ray sources

Details Infrared studies of X-ray sources Infrared studies of X-ray sources

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.102..359a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 102, no. 2, July 1984, p. 359-366. Research supported by the Department of

Astronomy and Astrophysics

Astronomy

Galactic Radiation, Infrared Astronomy, Milky Way Galaxy, X Ray Sources, Eclipsing Binary Stars, Frequency Distribution, Galactic Bulge, Neutron Stars, Radiant Flux Density

Scientific paper

A detailed study of the infrared radiation from galactic X-ray sources indicates that the galactic bulge sources and X-ray binary sources have different infrared emission characteristics. The galactic bulge sources seem to show a power law dependence between the X-ray flux and the infrared flux emitted by the X-ray source. The results presented suggest that the infrared radiation in the galactic bulge sources is dominated by free-free radiation and, in the case of eclipsing binary sources, the black-body emission from the early-type companion star contributes significantly to the infrared radiation.

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