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9.17. Accretion disk winds driven by the disk radiation field under radiation drag

Published online by Cambridge University Press:  25 May 2016

Y. Tajima  and
J. Fukue
Y. Tajima
Affiliation:
Astronomical Institute, Osaka Kyoiku University, Asahigaoka, Kashiwara, Osaka 582, Japan
J. Fukue
Affiliation:
Astronomical Institute, Osaka Kyoiku University, Asahigaoka, Kashiwara, Osaka 582, Japan

Extract

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The radiative winds from a geometrically thin accretion disk are studied. The effect of radiation drag which causes in the intense radiation fields around the accretion disk is examined recently. Then, we numerically consider the radiatively-accelerated accretion-disk winds which consist of ionized gas particles, taking into account radiation drag of the order of v/c.

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. 415 - 416
Copyright
Copyright © Kluwer 1998 

References

Tajima, Y., Fukue, J. (1997) Radiative Disk Winds under Radiation Drag II : Full Treatment, PASJ, submitted.CrossRefGoogle Scholar