Hostname: page-component-5c6d5d7d68-sv6ng Total loading time: 0 Render date: 2024-08-23T03:20:36.820Z Has data issue: false hasContentIssue false
  • English
  • Français

Quasars, supermassive black holes, and host galaxy evolution

Published online by Cambridge University Press:  01 December 2004

Fred Hamann ,
Craig Warner  and
Matthias Dietrich
Fred Hamann
Affiliation:
Department of Astronomy, University of Florida, Gainesville, FL 32611-2055, USA
Craig Warner
Affiliation:
Department of Astronomy, University of Florida, Gainesville, FL 32611-2055, USA
Matthias Dietrich
Affiliation:
Department of Physics and Astronomy, Georgia State University, 29 Peachtree Center Avenue, Science Annex, Suite 400, Atlanta, GA 30303-4106, 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.

We discuss some recent results from a program to study the relationships between AGNs, super-massive black holes (SMBHs), and their surrounding host galaxies. The results are based on broad emission-line diagnostics of the SMBH masses and metal abundances in a unique sample of 578 Type 1 AGNs.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
ORAL CONTRIBUTIONS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 489 - 492
Copyright
© 2004 International Astronomical Union