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X-ray Observations of SN 1993J

  • H.-U. Zimmermann
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

Summary

In April 2001 SN1993J was observed with both the PN and MOS cameras of the XMM-Newton observatory. A 2-component thermal emission model assuming ionization equilibrium provides a good fit to the spectrum in the 0.3 to 11 keV energy band, but fits to shock models show also acceptable results. The development of the X-ray temperatures over the first 8 years after the explosion is discussed in the light of the standard SN model. The long term X-ray lightcurve shows a general decline of the luminosity with L x α t −0.30.

Keywords

Reverse Shock High Temperature Component Forward Shock Progenitor Star Circumstellar Matter 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • H.-U. Zimmermann
    • 1
  1. 1.Max-Planck-Institut für extraterrestrische PhysikGarchingGermany

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