Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-29T10:21:06.219Z Has data issue: false hasContentIssue false
  • English
  • Français

M-σ relation in radio-loud AGNs and NLS1s

Published online by Cambridge University Press:  24 November 2004

W. Bian  and
Y. Zhao
W. Bian
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China Department of Physics, Nanjing Normal University, Nanjing 210097, China
Y. Zhao
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
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.

There is a tight M−σ relation in nearby inactive galaxies. Nearby radio-quiet AGNs also followed this relation. In order to investigate whether radio-loud AGNs and NLS1s follow this relation or not, we estimated their central black hole masses from Hβ and the bulge velocity dispersions from [O III] linewidth. We found that radio-loud AGNs and NLS1s seemed to deviate from this relation.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 79 - 80
Copyright
© 2004 International Astronomical Union