PRESUPERNOVA EVOLUTION OF MASSIVE STARS

被引:428
作者
NOMOTO, K
HASHIMOTO, M
机构
[1] BROOKHAVEN NATL LAB,DEPT PHYS,UPTON,NY 11973
[2] MAX PLANCK INST ASTROPHYS,D-8046 GARCHING,FED REP GER
来源
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 1988年 / 163卷 / 1-3期
关键词
D O I
10.1016/0370-1573(88)90032-4
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
引用
收藏
页码:13 / 36
页数:24
相关论文
共 48 条
[1]  
ARNETT WD, 1978, PHYSICS ASTROPHYSICS, P356
[2]   STARS IN MASS RANGE 7 LESS-THAN OR APPROXIMATELY EQUAL TO M/M PERIOD LESS-THAN OR APPROXIMATELY EQUAL TO 10 AS CANDIDATES FOR PULSAR PROGENITORS [J].
BARKAT, Z ;
REISS, Y ;
RAKAVY, G .
ASTROPHYSICAL JOURNAL, 1974, 193 (01) :L21-L23
[3]   COLLAPSE OF 9 M. STARS [J].
BARON, E ;
COOPERSTEIN, J ;
KAHANA, S .
ASTROPHYSICAL JOURNAL, 1987, 320 (01) :300-303
[4]  
BARON E, 1987, PREPRINT
[5]  
BERTELLI G, 1985, ASTRON ASTROPHYS, V150, P33
[6]   SUPER-NOVA THEORY [J].
BROWN, GE ;
BETHE, HA ;
BAYM, G .
NUCLEAR PHYSICS A, 1982, 375 (03) :481-532
[7]   THE PROMPT MECHANISM OF TYPE-II SUPERNOVAE [J].
BURROWS, A ;
LATTIMER, JM .
ASTROPHYSICAL JOURNAL, 1985, 299 (01) :L19-L22
[8]   TABLES OF THERMONUCLEAR REACTION-RATES FOR LOW-MASS NUCLEI C1 LESS-THAN-OR-EQUAL-TO Z LESS-THAN-OR-EQUAL-TO 14) [J].
CAUGHLAN, GR ;
FOWLER, WA ;
HARRIS, MJ ;
ZIMMERMAN, BA .
ATOMIC DATA AND NUCLEAR DATA TABLES, 1985, 32 (02) :197-233
[9]   A COMPARATIVE-STUDY OF SUPERNOVA LIGHT CURVES [J].
DOGGETT, JB ;
BRANCH, D .
ASTRONOMICAL JOURNAL, 1985, 90 (11) :2303-2311