Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources

Details Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources

2011-01-24

arxiv.org/abs/1101.4626v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

4 pages including a figure; to appear in the proceedings of MG12, Marcel Grossman Meeting, Paris, France, 12-18 July 2009

Scientific paper

We model two temperature viscous accretion flows in the sub-Keplerian,
optically thin, regime around rotating black holes including important
radiation effects self-consistently. The model successfully explains observed
luminosities from ultra-luminous to under-luminous sources and predicts the
spin parameter of black holes.

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