paper

Advection Dominated Accretion Flows Around Kerr Black Holes

arXiv:astro-ph/9607021 · doi:10.1086/178004

Abstract

We derive all relevant equations needed for constructing a global general relativistic model of advectively cooled, very hot, optically thin accretion disks around black holes and present solutions which describe advection dominated flows in the gravitational field of a Kerr black hole.

ApJ submitted

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