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Optical to X-rays SNe light curves following shock breakout through a thick wind

Published online by Cambridge University Press:  05 September 2012

Gilad Svirski ,
Ehud Nakar  and
Re'em Sari
Gilad Svirski
Affiliation:
Raymond and Beverly Sackler School of Physics & Astronomy, Tel Aviv University, Tel Aviv 69978, Israel
Ehud Nakar
Affiliation:
Raymond and Beverly Sackler School of Physics & Astronomy, Tel Aviv University, Tel Aviv 69978, Israel
Re'em Sari
Affiliation:
Racah Institute for Physics, The Hebrew University, Jerusalem 91904, Israel
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Abstract

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We present luminosity and temperature light curves following supernova shock breakouts through a thick wind. These events are very luminous and their spectrum may contain both an X-ray and a UV/optical component. For breakout pulse durations between a week and a month, the X-ray component luminosity peaks 100-500 days after the explosion, respectively.

Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 399 - 400
Copyright
Copyright © International Astronomical Union 2012

References

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