ON THE COMPOSITION OF THE STELLAR WINDS OF THE MOST MASSIVE STAR - 100 M. TO 2200 M.

被引:20
作者
DEARBORN, DSP
BLAKE, JB
机构
[1] UNIV ARIZONA,STEWARD OBSERV,TUCSON,AZ 85724
[2] AEROSPACE CORP,SPACE SCI LAB,LOS ANGELES,CA 90009
关键词
D O I
10.1086/161748
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:783 / 790
页数:8
相关论文
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[2]  
ALLEN DA, 1972, ASTRON ASTROPHYS, V20, P333
[3]  
ANDERSON MR, 1980, NUCL PHYS A, V349, P157
[4]  
Arnett W. D., 1973, EXPLOSIVE NUCLEOSYNT, P236
[5]   AL-26 PRODUCTION FROM A STELLAR EVOLUTIONARY SEQUENCE [J].
ARNETT, WD ;
WEFEL, JP .
ASTROPHYSICAL JOURNAL, 1978, 224 (03) :L139-L142
[6]  
ARNETT WD, 1972, AP J, V140, P499
[7]   SYNTHESIS OF AL-26 IN EXPLOSIVE HYDROGEN BURNING [J].
ARNOULD, M ;
NORGAARD, H ;
THIELEMANN, FK ;
HILLEBRANDT, W .
ASTROPHYSICAL JOURNAL, 1980, 237 (03) :931-950
[8]   NUCLEOSYNTHESIS OF NEUTRON-RICH HEAVY-NUCLEI DURING EXPLOSIVE HELIUM BURNING IN MASSIVE STARS [J].
BLAKE, JB ;
WOOSLEY, SE ;
WEAVER, TA ;
SCHRAMM, DN .
ASTROPHYSICAL JOURNAL, 1981, 248 (01) :315-320
[9]   LOCAL GAMMA-RAYS AND COSMIC-RAY ACCELERATION BY SUPERSONIC STELLAR WINDS [J].
CASSE, M ;
PAUL, JA .
ASTROPHYSICAL JOURNAL, 1980, 237 (01) :236-243
[10]  
CASSE M, 1981, ORIGIN COSMIC RAYS, P35