Hostname: page-component-8448b6f56d-t5pn6 Total loading time: 0 Render date: 2024-04-25T06:09:51.916Z Has data issue: false hasContentIssue false
  • English
  • Français

Dusty Structure Around Type 1 AGNs

Published online by Cambridge University Press:  03 June 2010

Rivay Mor ,
Hagai Netzer  and
Moshe Elitzur
Rivay Mor
Affiliation:
Tel-Aviv University, Tel-Aviv 69978, Israel Email: rivay@wise.tau.ac.il
Hagai Netzer
Affiliation:
Tel-Aviv University, Tel-Aviv 69978, Israel Email: rivay@wise.tau.ac.il
Moshe Elitzur
Affiliation:
University of Kentucky, Lexington, KY 40506-0055, 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 present a detailed investigation of the MIR continuum emission of type 1 QSOs and define the main emission components. Our model requires three components: a clumpy torus, dusty narrow-line region (NLR) clouds and a blackbody-like hot dust.

Keywords

galaxies: activequasars: 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. 125
Copyright
Copyright © International Astronomical Union 2010

References

Mor, R., Netzer, H., & Elitzur, M. 2009, ApJ, 705, 298CrossRefGoogle Scholar
Nenkova, M., Sirocky, M. M., Ivezić, Ž., & Elitzur, M. 2008, ApJ, 685, 147CrossRefGoogle Scholar