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APT4 - Astrophysical Black Holes from Quasars to Nano-Quasars

Speaker

Mukhopadhyay, Banibrata

Talk Title

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

Abstract

We model two temperature viscous accretion flows in the sub-Keplerian regime around rotating black holes. The model successfully explains observed luminosities from ultra- to under-luminous sources and predicts the spin frequency of black holes.

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