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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

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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

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