Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-25T16:40:14.783Z Has data issue: false hasContentIssue false
  • English
  • Français

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
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 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

Chevalier, R. A. & Irwin, C. M. 2012, ApJL, 747, L17CrossRefGoogle Scholar
Katz, B., Budnik, R., & Waxman, E. 2010, ApJ, 716, 781CrossRefGoogle Scholar
Katz, B., Sapir, N., & Waxman, E. 2011, ArXiv e-printsGoogle Scholar
Nakar, E. & Sari, R. 2010, ApJ, 725, 904CrossRefGoogle Scholar
Ofek, E. O., et al. 2010, ApJ, 724, 1396CrossRefGoogle Scholar
Svirski, G., Nakar, E., & Sari, R. 2012, ArXiv e-printsGoogle Scholar
Weaver, T. A. 1976, ApJS, 32, 233CrossRefGoogle Scholar