A CALCULATION OF A WHITE DWARF SUPERNOVA

被引:68
作者
HANSEN, CJ
WHEELER, JC
机构
[1] Joint Institute for Laboratory Astrophysics, Boulder, Colo.
关键词
D O I
10.1007/BF00653366
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A hydrodynamic calculation of a 1.42 M⊙ white dwarf supernova is described. Instability and collapse are initiated by electron capture and the subsequent nuclear detonation of C12 at high densities is sufficient to disperse all the material of the star with an average velocity of 7000 km/sec © 1969 D. Reidel Publishing Company.
引用
收藏
页码:464 / &
相关论文
共 34 条
[1]  
ALLER LH, 1964, STELLAR STRUCTURE ED, pCH2
[2]  
[Anonymous], 1965, Mem. RAS
[3]  
Arnett W.D., 1967, Canadian Journal of Physics, V45, P1621
[4]   GRAVITATIONAL COLLAPSE AND WEAK INTERACTIONS [J].
ARNETT, WD .
CANADIAN JOURNAL OF PHYSICS, 1966, 44 (11) :2553-+
[5]  
BAGLIN A, 1967, ANN ASTROPHYS, V30, P617
[6]  
Baglin A., 1968, Astrophysical Letters, V1, P143
[7]   ELECTRON CAPTURE IN STELLAR INTERIORS [J].
BAHCALL, JN .
ASTROPHYSICAL JOURNAL, 1964, 139 (01) :318-+
[8]   NUCLEOSYNTHESIS DURING SILICON BURNING [J].
BODANSKY, D ;
CLAYTON, DD ;
FOWLER, WA .
PHYSICAL REVIEW LETTERS, 1968, 20 (04) :161-&
[9]  
CHANDRASEKHAR S, 1939, INTRODUCTION STUDY S
[10]   HYDRODYNAMIC BEHAVIOR OF SUPERNOVAE EXPLOSIONS [J].
COLGATE, SA ;
WHITE, RH .
ASTROPHYSICAL JOURNAL, 1966, 143 (03) :626-&