ON THE CORRELATION OF CO LINE AND RADIO-CONTINUUM EMISSION IN NEARBY GALAXIES AND THE EFFICIENCY OF OB STAR FORMATION

被引:22
作者
ISRAEL, FP [1 ]
ROWANROBINSON, M [1 ]
机构
[1] UNIV LONDON QUEEN MARY COLL,DEPT APPL MATH,LONDON E1 4NS,ENGLAND
关键词
D O I
10.1086/162276
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
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页码:81 / 89
页数:9
相关论文
共 57 条
[1]  
ALLEN RJ, 1978, ASTRON ASTROPHYS, V62, P397
[2]  
ALLEN RJ, 1972, ASTRON ASTROPHYS, V19, P317
[3]  
BERKHUIJSEN EM, 1974, ASTRON ASTROPHYS, V34, P173
[4]   CO EMISSION FROM SEYFERT-GALAXIES [J].
BIEGING, JH ;
BLITZ, L ;
LADA, CJ ;
STARK, AA .
ASTROPHYSICAL JOURNAL, 1981, 247 (02) :443-448
[5]   THE LARGEST H-II-REGIONS IN M101 [J].
BLITZ, L ;
ISRAEL, FP ;
NEUGEBAUER, G ;
GATLEY, I ;
LEE, TJ ;
BEATTIE, DH .
ASTROPHYSICAL JOURNAL, 1981, 249 (01) :76-82
[6]  
BLITZ L, 1982, EXTRAGALACTIC MOL
[7]  
BLITZ L, 1978, NASA TM79708
[8]  
BOSMA A, 1982, ASTR AP S, V54, P387
[9]  
BOULANGER F, 1981, ASTRON ASTROPHYS, V93, pL1
[10]  
COMBES F, 1978, ASTRON ASTROPHYS, V67, pL13