Optical, UV and X-ray observations of X-ray binaries

Details Optical, UV and X-ray observations of X-ray binaries Optical, UV and X-ray observations of X-ray binaries

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.239...99b&link_type=abstract

In ESA Proceedings of ESA Workshop on a Cosmic X-Ray Spectroscopy Mission p 99-106 (SEE N86-22461 12-89)

Astronomy and Astrophysics

Astronomy

Stellar Spectrophotometry, Ultraviolet Astronomy, X Ray Astronomy, X Ray Binaries, Accretion Disks, H Ii Regions, Magellanic Clouds, Milky Way Galaxy

Scientific paper

The authors have observed a number of X-ray binary candidates in the Galaxy and in the Magellanic Clouds in the optical, far ultraviolet and X-ray bands. They present preliminary results on two sources for which the photometric and spectroscopic data suggest the presence of an accretion disk. For another source (LMC X-1) the authors show several observational evidences of interaction of the strong X-ray source with the surrounding H II region and the discovery of an X-ray ionized He III region.

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