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The Evolving XUV Absorber in NGC 3516

Published online by Cambridge University Press:  12 April 2016

Smita Mathur ,
Belinda Wilkes  and
Thomas Aldcroft
Smita Mathur
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Belinda Wilkes
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Thomas Aldcroft
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA

Abstract

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For NGC 3516 we find that the X-ray warm absorption and the broad UV associated absorption features can be produced by the same absorbing material. We argue that the evolution of the XUV absorber from pre-1992 to 1995 is consistent with expectation for an expanding, outflowing material.

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. 234 - 235
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Ferland, G.F. 1991 ‘HAZY’, OSU Astronomy Department Internal Report.Google Scholar
Kriss, G., et al. 1996, ApJL, in press.Google Scholar
Koratkar, A., et al. 1996, ApJ, in press.Google Scholar
Mathur, S., Wilkes, B., Elvis, M. & Fiore, F. 1994, ApJ, 434, 493.Google Scholar
Mathur, S., Elvis, M., & Wilkes, B. 1995, ApJ, 452, 230.CrossRefGoogle Scholar