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Associated Absorption at Low and High Redshift

Published online by Cambridge University Press:  12 April 2016

Martin Elvis
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Smita Mathur
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Belinda J. Wilkes
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Fabrizio Fiore
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA SAX Data Center, Roma, Italy
Paolo Giommi
Affiliation:
SAX Data Center, Roma, Italy
Paolo Padovan
Affiliation:
SAX Data Center, Roma, Italy
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Abstract

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Combining information on absorbing material in AGN from X-ray and the UV creates a powerful investigative tool. Here we give examples from both low and high redshift.

Type
V. Emission Lines, Absorption Lines, the Continuum, and their Relationships
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

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Associated Absorption at Low and High Redshift
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