Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-27T21:26:55.494Z Has data issue: false hasContentIssue false
  • English
  • Français

Investigating the High-Luminosity End of the Active Galaxy MBH–σ* Relation

Published online by Cambridge University Press:  03 June 2010

C. J. Grier ,
L. C. Watson ,
B. M. Peterson ,
P. Martini ,
M. C. Bentz ,
K. M. Dasyra ,
K. D. Denney ,
M. Dietrich ,
L. Ferrarese  and
R. W. Pogge
...Show all authors
C. J. Grier
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA Email: [email protected]
L. C. Watson
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA Email: [email protected]
B. M. Peterson
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA Email: [email protected] Center for Cosmology & AstroParticle Physics, The Ohio State University
P. Martini
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA Email: [email protected] Center for Cosmology & AstroParticle Physics, The Ohio State University
M. C. Bentz
Affiliation:
Department of Physics and Astronomy, University of California at Irvine
K. M. Dasyra
Affiliation:
Spitzer Science Center, California Institute of Technology
K. D. Denney
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA Email: [email protected]
M. Dietrich
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA Email: [email protected]
L. Ferrarese
Affiliation:
Herzberg Institute of Astrophysics, National Research Council of Canada
R. W. Pogge
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA Email: [email protected] Center for Cosmology & AstroParticle Physics, The Ohio State University
L. J. Tacconi
Affiliation:
Max Planck Institut fur extraterrestrische Physik
Rights & Permissions [Opens in a new window]

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.

While characterization of the MBH–σ* relationship in AGNs has improved due to the increase in available data and the improvement in accuracy of both MBH and σ* measurements, additional data at the high-luminosity end of the distribution of quasars are needed, as recent studies indicate that perhaps the relation steepens in this regime. To this end, we present three new measurements in objects at the high-luminosity end of the relation.

Keywords

galaxies: activegalaxies: nucleiquasars: emission lines
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. 204
Copyright
Copyright © International Astronomical Union 2010

References

Dasyra, K. M., et al. 2008, ApJ, 657, 102CrossRefGoogle Scholar
Grier, C. J., et al. 2008, ApJ, 688, 837CrossRefGoogle Scholar
Tremaine, S., et al. 2002, ApJ, 574, 740CrossRefGoogle Scholar
Onken, C. A., et al. 2004, ApJ, 615, 645CrossRefGoogle Scholar
Watson, L. C., et al. 2008, ApJ, 682, 21CrossRefGoogle Scholar