2002/12/30 by S. I. Blinnikov, D. K. Nadyozhin, S. E. Woosley +1
Physics and Astronomy · #astro-ph
published as "Nuclear Astrophysics", W.Hillebrandt and Ewald Mueller (Eds.), MPA 2002, p. 144 - 147 · 4 pages 4 figures. 11th Workshop on "Nuclear Astrophysics", Ringberg Castle, Tegernsee, Germany, February 11-16, 2002. Minor corrections
arxiv created 2002/12/30 · arxiv updated 2009/12/01
Numerical modeling of shock breakout in compact presupernovae of type Ib/c is done by two independent methods. Peak color temperatures reach 4 to 8 million K for explosion energies 1 to 9 foe with a typical local time-scale of 0.03 seconds. In the obverver's frame the burst is smeared over few seconds due to light travel time correction R/c.