SENSITIVITY OF STAR FORMATION RATE TO INTERSTELLAR GAS ABUNDANCE OF HEAVY ELEMENTS

被引：32

作者：

TALBOT, RJ

机构：

[1] INST ASTRON,CAMBRIDGE,ENGLAND

[2] RICE UNIV,DEPT SPACE PHYS & ASTRON,HOUSTON,TX 77001

来源：

ASTROPHYSICAL JOURNAL | 1974年 / 189卷 / 02期

关键词：

D O I：

10.1086/152790

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：209 / 215

页数：7

共 37 条

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[19] SPECTROPHOTOMETRIC RESULTS FROM COPERNICUS-SATELLITE .2. COMPOSITION OF INTERSTELLAR CLOUDS [J].

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