Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-22T02:45:18.043Z Has data issue: false hasContentIssue false
  • English
  • Français

The extremes of (X-ray) variability among galaxies: Flares from stars tidally disrupted by supermassive black holes

Published online by Cambridge University Press:  24 November 2004

S. Komossa
S. Komossa
Affiliation:
Max-Planck-Institut fuer extraterrestrische Physik, Giessenbachstr., 85748 Garching, Germany email: skomossa@mpe.mpg.de
Rights & Permissions [Opens in a new window]

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.

We discuss follow-up X-ray observations of giant-amplitude, non-recurrent X-ray flares, interpreted as tidal disruptions of stars by supermassive black holes at the centers of the flaring galaxies. The flare observations open up a new window to study supermassive black holes and their environment, and the physics of accretion events, in non-active galaxies.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
ORAL CONTRIBUTIONS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 45 - 48
Copyright
© 2004 International Astronomical Union