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SMBH Luminosity in the Starburst Environment

Published online by Cambridge University Press:  03 June 2010

Sergiy Silich ,
Guillermo Tenorio-Tagle ,
Filiberto Hueyotl-Zahuantitla ,
Jan Palouš  and
Richard Wünsch
Sergiy Silich
Affiliation:
Instituto Nacional de Astrofí sica Optica y Electrónica, Puebla, México
Guillermo Tenorio-Tagle
Affiliation:
Instituto Nacional de Astrofí sica Optica y Electrónica, Puebla, México
Filiberto Hueyotl-Zahuantitla
Affiliation:
Instituto Nacional de Astrofí sica Optica y Electrónica, Puebla, México
Jan Palouš
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, Prague, Czech Republic
Richard Wünsch
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, Prague, Czech Republic
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We claim that in the starburst environment there is no accretion of the ISM onto the BH and thus, in such cases, the BH luminosity is regulated by the mass-loss rate from massive stars in the star forming region. We calculate the accretion rate and show that it is usually small during the superwind stage and grows at the post-starburst stage, when the matter reinserted by intermediate–mass stars remains gravitationally bound and fuels the central BH.

Keywords

galaxies: Seyfertgalaxies: starburstaccretionhydrodynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 336
Copyright
Copyright © International Astronomical Union 2010

References

Davies, R. I., et al. 2007, ApJ, 671, 1388CrossRefGoogle Scholar
Silich, S., Tenorio-Tagle, G., & Hueyotl-Zahuantitla, F. 2008, ApJ, 686, 172CrossRefGoogle Scholar