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Optical Observations of X-Ray Binaries

Published online by Cambridge University Press:  30 March 2016

J.B. Hutchings
J.B. Hutchings*
Affiliation:
Dominion Astrophysical Observatory

Extract

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Recent progress in identifying the optical counterparts of X-ray sources has been slow, mostly because candidates are faint and X-ray data show no periodicities by which the identification can be confirmed. This report therefore deals with the investigation of some candidates to seek confirmation of their identity with the X-ray emitters, as well as details which are new or important concerning the few known binary sources. I shall also make some general remarks on the properties of the sources as they now appear, but leave a critical assessment of the masses to the next speaker.

Type
Joint Dicussions
Information
Highlights of Astronomy , Volume 4 , Issue 1: Highlights of Astronomy. As presented at the XVIth General Assembly of the IAU, 1976 (Part I) , 1977 , pp. 129 - 136
Copyright
Copyright © Reidel 1977

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