Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-13T15:11:26.510Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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