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11.9. Jets from time-dependent accretion flows onto a black hole

Published online by Cambridge University Press:  25 May 2016

Koji Nobuta  and
Tomoyuki Hanawa
Koji Nobuta
Affiliation:
Department of Astrophysics, School of Science, Nagoya University, Chikusa-ku, Nagoya 464-01, Japan
Tomoyuki Hanawa
Affiliation:
Department of Astrophysics, School of Science, Nagoya University, Chikusa-ku, Nagoya 464-01, Japan

Extract

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It is widely believed that accretion onto a black hole is the origin of X- and γ-ray emission and jets emerging from AGNs. Since the X- and γ-rays are highly variable, the accretion is also expected to be variable. We investigate highly variable hydrodynamical accretion with numerical simulations.

Type
Part III. Black Holes and Central Activity
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 473 - 474
Copyright
Copyright © Kluwer 1998 

References

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Nobuta, K. & Hanawa, T. 1997, ApJ, submitted.Google Scholar