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The relation between the properties of the NLR in narrow-line Seyfert 1 galaxies and the accretion rate

Published online by Cambridge University Press:  01 August 2006

Dawei Xu  and
Stefanie Komossa
Dawei Xu
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China email: dwxu@bao.ac.cn
Stefanie Komossa
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany email: skomossa@mpe.mpg.de
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Abstract

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We present a systematic study of the properties of the narrow-line region (NLR) of narrow-line Seyfert 1 galaxies (NLS1s) using Sloan Digital Sky Survey (SDSS) spectroscopy. Various correlations between the observed parameters and physical properties of NLS1s and broad-line Seyfert 1 galaxies (BLS1s) are detected. We search for possible origins of these trends by employing correlation analyses. We further investigate the relationship between black hole mass, Eddington ratio (L/LEdd) and physical parameters of the NLR.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S238: Black Holes from Stars to Galaxies – Across the Range of Masses , August 2006 , pp. 473 - 474
Copyright
Copyright © International Astronomical Union 2007

References

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