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Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources
Published 24 Jan 2011 in astro-ph.HE and gr-qc | (1101.4626v1)
Abstract: 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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