Abstract
We simulate shock propagation in a wide range of core-collapsing presupernovae: from compact WR stars exploding as SNe Ib/c through very extended envelopes of the narrow-line SNe IIn. We find that the same physical phenomenon of radiating shocks can produce outbursts of X-ray radiation (with photon energy $3kT sim 1 keV) lasting only a second in SNe Ib/c, as well as a very high flux of visual light, lasting for months, in SNe IIn.
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CITATION STYLE
Blinnikov, S., Chugai, N., Lundqvist, P., Nadyozhin, D., Woosley, S., & Sorokina, E. (2006). Observable Effects of Shocks in Compact and Extended Presupernovae. In From Twilight to Highlight: The Physics of Supernovae (pp. 23–26). Springer-Verlag. https://doi.org/10.1007/10828549_4
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