Hostname: page-component-669899f699-g7b4s Total loading time: 0 Render date: 2025-04-25T22:33:08.683Z Has data issue: false hasContentIssue false
  • English
  • Français

Supermassive black holes from OASIS and SAURON integral-field kinematics

Published online by Cambridge University Press:  01 July 2007

Michele Cappellari ,
R. Bacon ,
Roger L. Davies ,
P. T. de Zeeuw ,
Eric Emsellem ,
Jesús Falcón-Barroso ,
Davor Krajnović ,
Harald Kuntschner ,
Richard M. McDermid  and
Reynier F. Peletier
...Show all authors
Michele Cappellari
Affiliation:
Sub-Department of Astrophysics, University of Oxford, U.K.
R. Bacon
Affiliation:
Univ. de Lyon 1, CRAL Observ. de Lyon; CNRS, Ecole Normale Supérieure de Lyon, France
Roger L. Davies
Affiliation:
Sub-Department of Astrophysics, University of Oxford, U.K.
P. T. de Zeeuw
Affiliation:
Sterrewacht Leiden, Leiden University, Leiden, The Netherlands
Eric Emsellem
Affiliation:
Univ. de Lyon 1, CRAL Observ. de Lyon; CNRS, Ecole Normale Supérieure de Lyon, France
Jesús Falcón-Barroso
Affiliation:
European Space and Technology Centre, Noordwijk, The Netherlands
Davor Krajnović
Affiliation:
Sub-Department of Astrophysics, University of Oxford, U.K.
Harald Kuntschner
Affiliation:
Space Telescope European Coordinating Facility, ESO, Garching, Germany
Richard M. McDermid
Affiliation:
Sterrewacht Leiden, Leiden University, Leiden, The Netherlands
Reynier F. Peletier
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands
Marc Sarzi
Affiliation:
Centre for Astrophysics Research, University of Hertfordshire, U.K.
Remco C. E. van den Bosch
Affiliation:
Sterrewacht Leiden, Leiden University, Leiden, The Netherlands
Glenn van de Ven
Affiliation:
Institute for Advanced Study, Princeton, USA
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.

Supermassive black holes are a key element in our understanding of how galaxies form. Most of the progress in this very active field of research is based on just ~30 determination of black hole masses, accumulated over the past decade. We illustrate how integral-field spectroscopy, and in particular our OASIS modeling effort can help improve the current situation.

Keywords

black hole physicsgalaxies: elliptical and lenticulargalaxies: kinematics and dynamicsgalaxies: nuclei
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S245: Formation and Evolution of Galaxy Bulges , July 2007 , pp. 215 - 218
Copyright
Copyright © International Astronomical Union 2008

References

Aller, M. C. & Richstone, D. O. 2007, ApJ, 665, 120Google Scholar
Cappellari, M. & McDermid, R. M., 2005, Class. Quantum Grav., 22, 347Google Scholar
Cappellari, M., et al. , 2006, MNRAS, 366, 1126CrossRefGoogle Scholar
de Zeeuw, P. T., et al. 2002, MNRAS, 329, 513CrossRefGoogle Scholar
Di Matteo, T., Springel, V., & Hernquist, L. 2005, Nature, 433, 604Google Scholar
Emsellem, E., et al. 2004, MNRAS, 352, 721CrossRefGoogle Scholar
Faber, S. M., et al. , 1997, AJ, 114, 1771Google Scholar
Ferrarese, L. & Merritt, D. 2000, ApJ, 539, L9Google Scholar
Ferrarese, L. 2002, ApJ, 578, 90Google Scholar
Ferrarese, L. & Ford, H. 2005, Space Science Reviews, 116, 523CrossRefGoogle Scholar
Gebhardt, K., et al. 2000, ApJ, 539, L13CrossRefGoogle Scholar
Gebhardt, K., et al. 2003, ApJ, 583, 92Google Scholar
Gebhardt, K., et al. 2007, ApJ, in press (arXiv:0709.0585v1 [astro-ph])Google Scholar
Graham, A. W., Erwin, P., Caon, N., & Trujillo, I. 2001, ApJ, 563, L11CrossRefGoogle Scholar
Häring, N. & Rix, H.-W. 2004, ApJ, 604, L89Google Scholar
Houghton, R. C. W., Magorrian, J., Sarzi, M., Thatte, N., Davies, R. L., & Krajnović, D. 2006, MNRAS, 367, 2CrossRefGoogle Scholar
Kormendy, J. & Richstone, D. 1995, ARA&A, 33, 581Google Scholar
Lauer, T. R., et al. 2007, ApJ, 664, 226Google Scholar
Magorrian, J., et al. 1998, AJ, 115, 2285Google Scholar
Marconi, A. & Hunt, L. K. 2003, ApJ, 589, L21Google Scholar
McDermid, R. M., et al. 2006, MNRAS, 373, 906CrossRefGoogle Scholar
Milosavljević, M. & Merritt, D. 2001, ApJ, 563, 34CrossRefGoogle Scholar
Milosavljević, M., Merritt, D., Rest, A., & van den Bosch, F. C. 2002, MNRAS, 331, L51CrossRefGoogle Scholar
Nowak, N., Saglia, R. P., Thomas, J., Bender, R., Pannella, M., Gebhardt, K., & Davies, R. I. 2007, MNRAS, 379, 909CrossRefGoogle Scholar
Pizzella, A., Corsini, E. M., Dalla Bontà, E., Sarzi, M., Coccato, L., & Bertola, F. 2005, ApJ, 631, 785CrossRefGoogle Scholar
Quinlan, G. D. & Hernquist, L. 1997, New Astronomy, 2, 533Google Scholar
Schwarzschild, M. 1979, ApJ, 232, 236Google Scholar
Shapiro, K. L., Cappellari, M., de Zeeuw, P. T., McDermid, R. M., Gebhardt, K., van den Bosch, R. C. E., & Statler, T. S., 2006, MNRAS, 370, 559CrossRefGoogle Scholar
Silk, J. & Rees, M. J. 1998, A&A, 331, L1Google Scholar
Tremaine, S., et al. 2002, ApJ, 574, 740Google Scholar