TY - GEN
T1 - Optical to X-rays SNe light curves following shock breakout through a thick wind
AU - Svirski, Gilad
AU - Nakar, Ehud
AU - Sari, Re'Em
PY - 2011/4
Y1 - 2011/4
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=84866239120&partnerID=8YFLogxK
U2 - 10.1017/S1743921312013531
DO - 10.1017/S1743921312013531
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AN - SCOPUS:84866239120
SN - 9781107019799
T3 - Proceedings of the International Astronomical Union
SP - 399
EP - 400
BT - Death of Massive Stars
PB - Cambridge University Press
ER -