Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-24T21:46:15.811Z Has data issue: false hasContentIssue false
  • English
  • Français

The Early Evolution of Massive Black Holes

Published online by Cambridge University Press:  03 June 2010

Marta Volonteri
Marta Volonteri*
Affiliation:
Astronomy Department, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, USA Email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

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.

Massive black holes (MBHs) are nowadays believed to reside in most local galaxies. Studies have also established a number of relations between the MBH mass and properties of the host galaxy such as bulge mass and velocity dispersion. These results suggest that central MBHs, while much less massive than their hosts (~ 0.1%), are linked to the evolution of galactic structure. When did it all start? In hierarchical cosmologies, a single big galaxy today can be traced back to the stage when it was split up in hundreds of smaller components. Did MBH seeds form with the same efficiency in small proto-galaxies, or did their formation have to await the buildup of substantial galaxies with deeper potential wells? I briefly review here some of the physical processes that are conducive to the evolution of the massive black hole population. I will discuss black hole formation processes for “seed” black holes that are likely to take place at early cosmic epochs, and possible observational tests of these scenarios.

Keywords

cosmology: theorygalaxies: formationgravitationblack hole physicsquasars: general
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. 26 - 33
Copyright
Copyright © International Astronomical Union 2010

References

Abel, T., Bryan, G. L., & Norman, M. L. 2000, ApJ, 540, 39CrossRefGoogle Scholar
Arun, K. G., Babak, S., Berti, E., Cornish, N., Cutler, C., Gair, J., Hughes, S. A., Iyer, B. R., Lang, R. N., Mandel, I., Porter, E. K., Sathyaprakash, B. S., Sinha, S., Sintes, A. M., Trias, M., Van Den Broeck, C., & Volonteri, M. 2009, Classical and Quantum Gravity, 26, 094027CrossRefGoogle Scholar
Barth, A. J., Ho, L. C., Rutledge, R. E., & Sargent, W. L. W. 2004, ApJ, 607, 90Google Scholar
Barth, A. J., Martini, P., Nelson, C. H., & Ho, L. C. 2003, ApJ, 594, L95Google Scholar
Baumgarte, T. W. & Shapiro, S. L. 1999, ApJ, 526, 941CrossRefGoogle Scholar
Begelman, M. C. 2009, MNRAS, in pressGoogle Scholar
Begelman, M. C. & Shlosman, I. 2009, ApJ, 702, L5CrossRefGoogle Scholar
Begelman, M. C., Volonteri, M., & Rees, M. J. 2006, MNRAS, 370, 289CrossRefGoogle Scholar
Bond, J. R., Arnett, W. D., & Carr, B. J. 1984, ApJ, 280, 825Google Scholar
Bromm, V., Coppi, P. S., & Larson, R. B. 1999, ApJ, 527, L5CrossRefGoogle Scholar
Bromm, V., Coppi, P. S., & Larson, R. B. 2002, ApJ, 564, 23CrossRefGoogle Scholar
Bromm, V. & Loeb, A. 2003, ApJ, 596, 34CrossRefGoogle Scholar
Clark, P. C., Glover, S. C. O., & Klessen, R. S. 2008, ApJ, 672, 757CrossRefGoogle Scholar
Devecchi, B. & Volonteri, M. 2009, ApJ, 694, 302CrossRefGoogle Scholar
Ferrarese, L. & Ford, H. 2005, Space Science Reviews, 116, 523CrossRefGoogle Scholar
Fryer, C. L., Woosley, S. E., & Heger, A. 2001, ApJ, 550, 372CrossRefGoogle Scholar
Gaburov, E., Lombardi, J., & Portegies Zwart, S. 2009 [arXiv0904.0997]Google Scholar
Glover, S. C. O., Clark, P. C., Greif, T. H., Johnson, J. L., Bromm, V., Klessen, R. S., & Stacy, A. 2008, in Open Questions in the Study of Population III Star Formation, eds. Hunt, L. K., Madden, S., & Schneider, R., (Cambridge: Cambridge University Press), p. 3Google Scholar
Gültekin, K., Richstone, D. O., Gebhardt, K., Lauer, T. R., Tremaine, S., Aller, M. C., Bender, R., Dressler, A., Faber, S. M., Filippenko, A. V., Green, R., Ho, L. C., Kormendy, J., Magorrian, J., Pinkney, J., & Siopis, C. 2009, ApJ, 698, 198CrossRefGoogle Scholar
Hoyle, F. & Fowler, W. A. 1963, MNRAS, 125, 169CrossRefGoogle Scholar
Kudritzki, R.-P. & Puls, J. 2000, ARAA, 38, 613Google Scholar
Lodato, G. & Natarajan, P. 2006, MNRAS, 371, 1813CrossRefGoogle Scholar
Madau, P. & Rees, M. J. 2001, ApJ, 551, L27CrossRefGoogle Scholar
McKee, C. F. & Tan, J. C. 2008, ApJ, 681, 771CrossRefGoogle Scholar
Omukai, K., Schneider, R., & Haiman, Z. 2008, ApJ, 686, 801CrossRefGoogle Scholar
Palla, F., Zinnecker, H., Maeder, A., & Meynet, G., eds. 2002, Physics of Star Formation in GalaxiesCrossRefGoogle Scholar
Peterson, B. M., Bentz, M. C., Desroches, L., Filippenko, A. V., Ho, L. C., Kaspi, S., Laor, A., Maoz, D., Moran, E. C., Pogge, R. W., & Quillen, A. C. 2005, ApJ, 632, 799Google Scholar
Rees, M. J., 1978, in Structure and Properties of Nearby Galaxies, eds. Berkhuijsen, E. M. & Wielebinski, R. (Dordrecht: Reidel), p. 237CrossRefGoogle Scholar
Saijo, M., Baumgarte, T. W., Shapiro, S. L., & Shibata, M. 2002, ApJ, 569, 349CrossRefGoogle Scholar
Santoro, F. & Shull, J. M. 2006, ApJ, 643, 26CrossRefGoogle Scholar
Schneider, R., Omukai, K., Inoue, A. K., & Ferrara, A. 2006, MNRAS, 369, 1437Google Scholar
Sesana, A., Volonteri, M., & Haardt, F., 2007, MNRAS, 377, 1711Google Scholar
Shapiro, S. L., 2004, in Coevolution of Black Holes and Galaxies, ed. Ho, L. C., (Cambridge: Cambridge University Press), p. 103Google Scholar
Shibata, M. & Shapiro, S. L. 2002, ApJ, 572, L39CrossRefGoogle Scholar
Shlosman, I., Frank, J., & Begelman, M. C. 1989, Nature, 338, 45CrossRefGoogle Scholar
Volonteri, M. & Gnedin, N. Y. 2009, ApJ, 703, 2113Google Scholar
Volonteri, M., Haardt, F., & Madau, P. 2003, ApJ, 582, 559CrossRefGoogle Scholar
Volonteri, M., Lodato, G., & Natarajan, P. 2008, MNRAS, 383, 1079Google Scholar
Volonteri, M. & Natarajan, P. 2009, MNRAS, 400, 1911Google Scholar
Yoshida, N., Omukai, K., Hernquist, L., & Abel, T. 2006, ApJ, 652, 6Google Scholar
Yu, Q. & Tremaine, S. 2002, MNRAS, 335, 965Google Scholar