Hostname: page-component-6bf8c574d5-zc66z Total loading time: 0 Render date: 2025-03-07T04:17:30.025Z Has data issue: false hasContentIssue false
  • English
  • Français

Accreting Plasmas in Black Hole Magnetospheres

Published online by Cambridge University Press:  25 May 2016

M. Takahashi
M. Takahashi*
Affiliation:
Department of Physics and Astronomy, Aichi University of Education, Kariya, Aichi 448-8542, Japan

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 present a fully relativistic study on the standing shock formation for magnetohydrodynamical plasmas in a stationary and axisymmetric black hole magnetosphere. We express all the postshock physical quantities in terms of the relativistic compression ratio. Then, the downstream state of a shocked plasma is determined by the upstream state of the accretion. We also discuss the dragging-effects of the rotating black hole on the shock conditions.

Type
Part I: Talks
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 233 - 240
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Appl, S., & Camenzind, M. 1988, A&A, 206, 258.Google Scholar
Bekenstein, J. D., & Oron, E. 1978, Phys. Rev. D, 18, 1809.CrossRefGoogle Scholar
Blandford, R. D., & Znajek, R. L. 1977, MNRAS, 179, 433.Google Scholar
Camenzind, M., 1986, A&A, 156, 137.Google Scholar
Rilett, D., Takahashi, M., Fukumura, K., & Tsuruta, S., in preparation.Google Scholar
Takahashi, M., 2000, in Proc. 19th Texas Symp. on Relativistic Astrophysics and Cosmology, eds. Aubourg, E., Montmerle, T., & Paul, J. (Paris: World Scientific Press), in press.Google Scholar