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3.24. Nuclear fueling by radiative avalanche induced by starbursts

Published online by Cambridge University Press:  25 May 2016

M. Umemura ,
Jun Fukue  and
Shin Mineshige
M. Umemura
Affiliation:
Center for Computational Physics, Tsukuba University, Tsukuba, Ibaraki 305, Japan; [email protected]
Jun Fukue
Affiliation:
Astronomical Institute, Osaka Kyoiku University, Asahigaoka, Kashiwara, Osaka 582, Japan; [email protected]
Shin Mineshige
Affiliation:
Department of Astronomy, Kyoto University, Sakyo-ku, Kyoto 606, Japan; [email protected]

Extract

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Recently, as a solid physical mechanism which links circumnuclear starbursts to AGN fueling, Umemura, Fukue, & Mineshige (1997a) have proposed a radiative avalanche which is the black hole accretion driven by intensive radiation from circumnuclear starbursts of ≲ 100 pc.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 137 - 138
Copyright
Copyright © Kluwer 1998 

References

Umemura, M., Fukue, J., Mineshige, S. (1997a) Radiative Avalanche: Starburst Induced Fuelling to AGNs, Astrophysical Journal Letters, Vol.479 no.2, pp. 97–100.Google Scholar
Umemura, M., Fukue, J., Mineshige, S. (1997b) Radiative Avalanche onto Galactic Nuclei Induced by Circumnuclear Starbursts, submitted to Astrophysical Journal .Google Scholar