Advection Dominated Accretion Flows Around Kerr Black Holes
Astrophysics
2009-10-28 v1
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.
Keywords
Cite
@article{arxiv.astro-ph/9607021,
title = {Advection Dominated Accretion Flows Around Kerr Black Holes},
author = {M. A. Abramowicz and X. -M. Chen and M. Granath and J. -P. Lasota},
journal= {arXiv preprint arXiv:astro-ph/9607021},
year = {2009}
}
Comments
ApJ submitted