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Supernova Fragments and the Origin of the Rapid X-ray Variability

Published online by Cambridge University Press:  19 July 2016

R. Cid Fernandes ,
R. Terlevich ,
G. Tenorio-Tagle ,
J. Franco  and
M. Rozyczka
R. Cid Fernandes
Affiliation:
Institute of Astronomy, Cambridge, U.K.
R. Terlevich
Affiliation:
Royal Greenwich Observatory, Cambridge, U.K.
G. Tenorio-Tagle
Affiliation:
Instituto de Astrofísica de Canarias, Tenerife, Spain
J. Franco
Affiliation:
Instituto de Astronomía UNAM, México D. F., México
M. Rozyczka
Affiliation:
Warsaw University Observatory, Warszaw, Poland

Abstract

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The Starburst model for Radio Quiet Active Galactic Nuclei proved able to explain the origin of the broad line region, the variability characteristics of line and continuum in Seyfert galaxies, X-ray spectra, the luminosity function of QSOs and etc. But can we understand the rapid X-ray variability observed in several AGN with supernovae?

Keywords

Active GalaxiesStarburstSupernova RemnantsX-ray
Type
Poster Contributions: X-Rays and Higher Energies
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 371
Copyright
Copyright © Kluwer 1994