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

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.

preprint2011arXivOpen access
Banibrata Mukhopadhyay
astro-ph.HEgr-qc
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Banibrata Mukhopadhyay

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