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Marginally stable thick discs orbiting the Kerr–de Sitter black holes: the mass estimates
Published online by Cambridge University Press: 01 August 2006
Abstract
Basic properties of equipotential surfaces in test perfect fluid tori with uniform distribution of the specific angular momentum orbiting KdS black holes are summarized. The central mass-densities of adiabatic non-relativistic tori, for which the approximation of test fluid is adequate, are given and compared with the typical densities of Giant Molecular Clouds.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S238: Black Holes from Stars to Galaxies – Across the Range of Masses , August 2006 , pp. 449 - 450
- Copyright
- Copyright © International Astronomical Union 2007