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Young X-ray-Emitting Supernovae in Galaxies

Published online by Cambridge University Press:  12 May 2006

Eric M. Schlegel
Eric M. Schlegel
Affiliation:
High Energy Astrophysics Division, Smithsonian Astrophysical Observatory, Cambridge, MA 02138 USA email: eschlegel@cfa.harvard.edu Department of Physics and Astronomy, University of Texas-San Antonio, San Antonio, TX 78249 USA email: eric_schlegel@utsa.edu
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Abstract

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This talk reviews the observations of the high-energy emission of young supernovae, providing an update from previous reviews in 1995 and 2003. A summary plot shows the number distribution of X-ray luminosities, currently totalling 25 supernovae, from which it is clear that SN IIP are weak X-ray sources, SN IIn are very luminous sources, and SN Ib/c cover a broad range in luminosity.

Keywords

supernovaesupernovae: individualX-rays: individualsupernova remnants
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S230: Populations of High Energy Sources in Galaxies , August 2005 , pp. 252 - 258
Copyright
2006 International Astronomical Union