Breakout of the supernova shock

被引：6

作者：

Bethe, HA

机构：

[1] Floyd R. Newman Laboratory of Nuclear Studies, Cornell University, Ithaca

来源：

ASTROPHYSICAL JOURNAL | 1996年 / 469卷 / 02期

关键词：

nuclear reactions; nucleosynthesis; abundances; shock waves; supernovae; general;

D O I：

10.1086/177822

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The shock in a supernova of Type II first moves slowly and then suddenly breaks out with a velocity of order 10(9) cm s(-1). This breakout is due to the recombination of nucleons into alpha-particles. It is shown that this recombination provides enough energy to lift the matter against gravity. The net energy after escape from the star is about 4 x 10(18) ergs g(-1). Supernovae of Type II differ mainly in the binding energy of the mantle of the progenitor.

引用

页码：737 / 739

页数：3

共 8 条

[1] THE SUPERNOVA SHOCK
BETHE, HA
[J]. ASTROPHYSICAL JOURNAL, 1995, 449 (02) : 714 - 726
[2] BETHE HA, 1993, APJ, V412, P1992
[3] A THEORY OF SUPERNOVA EXPLOSIONS
BURROWS, A
GOSHY, J
[J]. ASTROPHYSICAL JOURNAL, 1993, 416 (02) : L75 - L78
[4] ON THE NATURE OF CORE-COLLAPSE SUPERNOVA EXPLOSIONS
BURROWS, A
HAYES, J
FRYXELL, BA
[J]. ASTROPHYSICAL JOURNAL, 1995, 450 (02) : 830 - &
[5] INSIDE THE SUPERNOVA - A POWERFUL CONVECTIVE ENGINE
HERANT, M
BENZ, W
HIX, WR
FRYER, CL
COLGATE, SA
[J]. ASTROPHYSICAL JOURNAL, 1994, 435 (01) : 339 - 361
[6] JANKA HT, 1995, ASTROPHYS J, V448, pL109, DOI 10.1086/309604
[7] WILSON JR, 1995, P 1994 M GROSSM M ST
[8] THE EVOLUTION AND EXPLOSION OF MASSIVE STARS .2. EXPLOSIVE HYDRODYNAMICS AND NUCLEOSYNTHESIS
WOOSLEY, SE
WEAVER, TA
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1995, 101 (01) : 181 - 235

← 1 →