A census of low mass black hole binaries
Roger W. Romani
Received 6 October 1997 / Accepted 16 January 1998
The six known low mass black hole binaries discovered as X-ray/Optical novae represent a relatively uniform source class. It is shown that the recurrence time for outbursts from these sources can be understood in the disk instability picture if magnetic braking is not active in the short period systems. An extrapolation from the discovery surveys gives an estimate of such systems in the Galaxy as a whole. BATSE sky monitor observations should produce new candidate black hole transients at a rate of /y. The population estimates also suggest that optical outbursts of black hole binaries prior to 1975 should have been recorded in classical nova catalogues. Some strategies for discovery of more black hole binaries are discussed.
Key words: black hole physics binaries: close novae, cataclysmic variables X-rays: stars Galaxy: stellar content
Send offprint requests to: R.W.Romani, Dept. of Physics, M.C. 4060, Stanford, CA 94350, USA
© European Southern Observatory (ESO) 1998
Online publication: April 20, 1998