Black hole accretion disks exhibiting superhumps

Details Black hole accretion disks exhibiting superhumps Black hole accretion disks exhibiting superhumps

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44l..15m&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 2, 1992, p. L15-L18. Research supported b

Statistics

Computation

41

Accretion Disks, Binary Stars, Black Holes (Astronomy), Stellar Mass, Computational Astrophysics, Ginga Satellite, Neutron Stars, Spaceborne Astronomy

Scientific paper

Two independent methods to derive the lower limits to the mass of a compact star in a cataclysmic system are introduced. If the superhumps in cataclysmic variables and in X-ray novae are of a common origin, the same methods can also be used in the case of X-ray sources. The methods are used to estimate the masses of the compact components in GS 2000 + 25 and GS 1124 - 68 at larger than 3.5 solar masses.

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