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A Multi-Wavelength Study of X-ray Selected AGN

Published online by Cambridge University Press:  07 August 2017

R. J. V. Brissenden ,
I. R. Tuohy ,
G. V. Bicknell ,
R. A. Remillard  and
D. A. Schwartz
R. J. V. Brissenden
Affiliation:
Mt. Stromlo and Siding Spring Observatories, the Australian National University, Private Bag, PO Woden, ACT 2606, Australia
I. R. Tuohy
Affiliation:
Mt. Stromlo and Siding Spring Observatories, the Australian National University, Private Bag, PO Woden, ACT 2606, Australia
G. V. Bicknell
Affiliation:
Mt. Stromlo and Siding Spring Observatories, the Australian National University, Private Bag, PO Woden, ACT 2606, Australia
R. A. Remillard
Affiliation:
Center for Space Research, MIT, Cambridge, MA 02139
D. A. Schwartz
Affiliation:
Harvard-Smithsonian CfA, 60 Garden Street, Cambridge, MA 02138

Extract

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A sample of Active Galactic Nuclei (AGN) have been discovered during a program to identify the optical counterparts of X-ray sources detected by the Modulation Collimator experiment of the High Energy Astronomy Observatory-1 (HEAO-1). UV-excess techniques were used to identify the X-ray sources (Remillard et al. 1986) and the details of the identifications are given elsewhere (Remillard et al. 1988, Brissenden et al. 1988). We report here the preliminary results of a multi-wavelength study of these new AGN.

Type
Part 3: X-rays and the Central Source
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 199 - 200
Copyright
Copyright © Kluwer 1989 

References

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