A summary of ongoing work on the properties, origin, and evolution of low-mass X-ray binaries in globular clusters and in the Galactic Bulge is presented. This discussion centers on the insights into these problems that can be derived from study of the ultracompact binary systems, such as the recently discovered 11-minute binary in the globular cluster NGC 6624.
Ultra-compact and X-ray binaries in globular clusters
Advances in Space Research ; 8 , 2-3
1988-01-01
Sonstige
Keine Angabe
Englisch
Ultra-compact and X-ray binaries in globular clusters
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