The extremely X-ray bright Wolf-Rayet star HD193793 |
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| Authors: | A M T Pollock |
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| Institution: | (1) Department of Space Research, University of Birmingham, P O Box 363, B15 2TT Birmingham, UK |
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| Abstract: | The Einstein Observatory showed that Wolf-Rayet stars have a much larger range in the ratio of X-ray to bolometric luminosity than normal early-type stars. EXOSAT measurements of HD193T93 (WCT+abs) show it to be extremely X-ray bright. This result is probably not connected with the infra-red and radio outburst that the star underwent in 1977. Other Einstein X-ray sources which are probably identified with Wolf-Rayet stars are newly reported. |
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