Hostname: page-component-848d4c4894-r5zm4 Total loading time: 0 Render date: 2024-06-19T03:07:45.192Z Has data issue: false hasContentIssue false
  • English
  • Français

A Correlation Analysis for Emission Lines in 52 AGN

Published online by Cambridge University Press:  12 April 2016

D. Dultzin-Hacyan ,
J. Sulentic ,
P. Marziani ,
M. Calvani  and
M. Moles
D. Dultzin-Hacyan
Affiliation:
Instituto de Astronomïa, UNAM, Méico D.F., México
J. Sulentic
Affiliation:
Department of Physics & Astronomy, University of Alabama, Tuscaloosa, AL 35487, USA
P. Marziani
Affiliation:
Osservatorio Astronomico, Padova, Italy
M. Calvani
Affiliation:
Osservatorio Astronomico, Padova, Italy
M. Moles
Affiliation:
Observatorio Astronómico Nacional, Madrid, Spain

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 recently completed the first comparison of high- and low-ionization broad lines in a sample of 52 AGN. We summarize here the principal results of a correlation analysis for this sample. We then briefly outline a model for the broad-line structure in radio-quiet AGN that is suggested by the correlation analysis.

Type
V. Emission Lines, Absorption Lines, the Continuum, and their Relationships
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 262 - 263
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Marziani, P., Sulentic, J.W., Dultzin-Hacyan, D., Calvani, M., & Moles, M. 1996, ApJS, 104, 37.Google Scholar
Sulentic, J.W., Marziani, P., Dultzin-Hacyan, D., Calvani, M., & Moles, M. 1995, ApJ, 445, L85.Google Scholar