Shock breakouts in SNe Ib/c

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dc.creatorBlinnikov, S. I.
dc.creatorNadyozhin, D. K.
dc.creatorWoosley, S. E.
dc.creatorSorokina, E. I.
dc.date2002-12-30
dc.date.accessioned2026-07-07T02:07:01Z
dc.date.available2026-07-07T02:07:01Z
dc.descriptionNumerical 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.
dc.description4 pages 4 figures. 11th Workshop on "Nuclear Astrophysics", Ringberg Castle, Tegernsee, Germany, February 11-16, 2002. Minor corrections
dc.identifierhttps://arxiv.org/abs/astro-ph/0212564
dc.identifierhttp://arxiv.org/abs/astro-ph/0212564
dc.identifier"Nuclear Astrophysics", W.Hillebrandt and Ewald Mueller (Eds.), MPA 2002, p. 144 - 147
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5563
dc.subjectAstrophysics
dc.titleShock breakouts in SNe Ib/c
dc.typetext

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