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Iron Lines, X-Rays, and Outflowing Winds

Published online by Cambridge University Press:  12 April 2016

A. Lawrence
A. Lawrence*
Affiliation:
Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK

Abstract

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The strength of optical Fe II lines seems to be connected to both X-ray spectral slope and X-ray loudness, as well as other interesting properties such as emission-line width and the presence of a low-ionization broad absorber. The reason for this cluster of correlations is far from clear.

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. 230 - 233
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Boroson, T.A., & Green, R.F. 1992, ApJS, 80, 109.Google Scholar
Boroson, T.A., & Meyers, K.A. 1992, ApJ, 397, 492.CrossRefGoogle Scholar
Gaskell, C.M. 1985, ApJ, 291, 112.Google Scholar
Joly, M. A&A, 242, 49.Google Scholar
Laor, A., Fiore, F., Elvis, M., Wilkes, B.J., & McDowell, J. 1994, ApJ, 435, 611.Google Scholar
Lawrence, A., Elvis, M., Wilkes, B.J., McHardy, I., & Brandt, N. 1996, MNRAS, submitted.Google Scholar
Norman, C., & Miley, G. 1984, A&A, 141, 85.Google Scholar
Weymann, R.J., Morris, S.L., Foltz, C.B., & Hewett, P.C. 1991, ApJ, 373, 23.Google Scholar
Wilkes, B.J., Elvis, M., & McHardy, I. 1988, ApJ, 353, 433.Google Scholar