Hostname: page-component-848d4c4894-2pzkn Total loading time: 0 Render date: 2024-05-07T04:07:16.167Z Has data issue: false hasContentIssue false

Can the Sonic Radius in ADAF Be Large?

Published online by Cambridge University Press:  25 May 2016

F. Yuan
Affiliation:
Astronomy Department, Nanjing University, Nanjing 210093, P.R.China
K.L. Huang
Affiliation:
Physics Department, Nanjing Normal University, Nanjing 210097, P.R.China
Ju-fu Lu
Affiliation:
Center for Astrophysics, University of Science and Technology of China, Hefei 230026, P.R.China

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We obtain the global transonic solutions by solving numerically a set of equations describing advection dominated accretion flows around black holes. We find that the sonic points can locate themselves at almost any radius, independent of the viscosity parameter α and the polytropic index γ.

Type
III. AGN Theory and Models
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Chakrabarti, S.K. 1996a, ApJ, 464, 664 (C96) CrossRefGoogle Scholar
Chakrabarti, S.K. 1996b, Physics Report, 266, No 5&6, 229 CrossRefGoogle Scholar
Chen, X., Abramowicz, M. A., & Lasota, J.-P. 1997, ApJ, 476, 61 (CAL) CrossRefGoogle Scholar
Igumenshchev, I. V., Abramowicz, M. A., & Novikov, I. D. 1998, MNRAS, 298, 1093 (IAN) CrossRefGoogle Scholar
Narayan, R., Kato, S. & Honma, F. 1997, ApJ, 476, 49 (NKH) CrossRefGoogle Scholar
Peitz, J. & Appl, S. 1997, MNRAS, 286, 681 (PA) CrossRefGoogle Scholar