Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-26T07:40:24.360Z Has data issue: false hasContentIssue false
  • English
  • Français

10.9. Dynamical constraints on alternatives to massive black holes in galactic nuclei

Published online by Cambridge University Press:  25 May 2016

Eyal Maoz
Eyal Maoz*
Affiliation:
Astronomy Department, University of California, Berkeley, CA 94720, USA

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

There is now compelling evidence for massive dark objects at the centers of severals galaxies. The possibility that these are black holes (BHs) fits well into the picture where quasars and AGNs are powered by accretion onto a massive BH, so that dead quasar engines should be hiding in many nearby galaxies.

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. 447 - 448
Copyright
Copyright © Kluwer 1998 

References

Kormendy, J. & Richstone, D. (1995), Inward Bound - The Search For Supermassive Black Holes in Galactic Nuclei, ARA&A, vol. 33, pp. 581–624.Google Scholar
Maoz, E. (1997) Dynamical Constraints On Alternatives To Massive Black Holes In Galactic Nuclei, submitted to ApJ .CrossRefGoogle Scholar