Globular cluster X ray binaries

Details Globular cluster X ray binaries Globular cluster X ray binaries

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..129c&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 129-137 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

7

Cataclysmic Variables, Globular Clusters, Star Distribution, X Ray Binaries, Exosat Satellite, Japanese Space Program, Stellar Luminosity, Stellar Mass, Stellar Spectra

Scientific paper

A review on recent observational progress on all the globular cluster X-ray sources, with emphasis on EXOSAT and Ginga results and associated ground based studies is given. It is known that the population of cluster sources divides into high and low Lx sources. The low Lx group itself divides into 2 subgroups of which the fainter sources were believed to be Cataclysmic Variables (CVs). No observational support can be found for this. Other programs to search for CVs in globular clusters are described.

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