MEAN MASS OF ABUNDANT COSMIC-RAY NUCLEI FROM BORON TO SILICON AT 1.2 GEV PER ATOMIC MASS UNIT

被引:35
作者
DWYER, R [1 ]
机构
[1] UNIV CHICAGO,DEPT PHYS,CHICAGO,IL 60637
关键词
D O I
10.1086/156417
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:691 / 707
页数:17
相关论文
共 42 条
[1]  
AGRAWAL PC, 1965, 9TH P INT COSM RAY C, V1, P453
[2]   ORIGIN OF COSMIC-RAYS, ATOMIC NUCLEI, AND PULSARS IN EXPLOSIONS OF MASSIVE STARS [J].
ARNETT, WD ;
SCHRAMM, DN .
ASTROPHYSICAL JOURNAL, 1973, 184 (02) :L47-L51
[3]  
BALASUBRAHMANYA.VK, 1963, 8TH P INT COSM RAY C, V3, P110
[4]  
BENEGAS JC, 1975, 14TH P INT C COSM RA, V1, P379
[5]  
BJARLE C, 1975, 14TH P INT COSM RAY, V1, P337
[6]  
CAMERON AGW, 1973, SPACE SCI REV, V15, P121, DOI 10.1007/BF00172440
[7]  
DAYTON B, 1969, DANISH SPACE RES I R
[8]   ISOTOPIC COMPOSITION OF COSMIC-RAY NITROGEN AT 1.5 GEV-AMU [J].
DWYER, R ;
MEYER, P .
PHYSICAL REVIEW LETTERS, 1975, 35 (09) :601-604
[9]   MEAN MASS OF COSMIC-RAY NE, MG, SI AT 1.2 GEV AMU-1 [J].
DWYER, R ;
MEYER, P .
ASTROPHYSICAL JOURNAL, 1977, 216 (02) :646-649
[10]  
Evenson P., 1975, 14TH P INT COSM RAY, V9, P3177