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Emission Line Properties of Seyfert 1 Type AGN from RASS

Published online by Cambridge University Press:  26 May 2016

D. W. Xu ,
S. Komossa ,
J. Y. Wei ,
X. Z. Zheng  and
Y. Qian
D. W. Xu
Affiliation:
Max-Plank-Institut für extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching, Germany National Astronomical Observatories, Beijing 100012, China
S. Komossa
Affiliation:
Max-Plank-Institut für extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching, Germany
J. Y. Wei
Affiliation:
National Astronomical Observatories, Beijing 100012, China
X. Z. Zheng
Affiliation:
National Astronomical Observatories, Beijing 100012, China
Y. Qian
Affiliation:
Tsinghua University, Beijing 100080, China

Abstract

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We present the optical emission line properties of a sample of 155 bright X-ray selected ROSAT Seyfert 1 type AGN. The measured properties are gathered for correlation analysis. The strong correlations between Hβ redshift, flux ratios of Fe II to Hβ broad component and [O III] to Hβ narrow component are found.

Type
Part 8 Active Galaxies and their Nuclei
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 273 - 274
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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