The physical state of the interstellar gas clouds

被引：7

作者：

Struve, O ^{[1
]}

机构：

[1] Univ Chicago, Yerkes Observ, Chicago, IL USA

来源：

PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA | 1939年 / 25卷

关键词：

D O I：

10.1073/pnas.25.1.36

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

引用

页码：36 / 43

页数：8

共 50 条

[21] ON PROCESSES OF GENESIS OF PROTOPLANETARY NEBULA FROM THE GAS-DUST INTERSTELLAR CLOUDS - PROCESSES IN INTERSTELLAR GAS
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[22] Physical state of molecular gas in high galactic latitude translucent clouds
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[23] INTERSTELLAR CLOUDS
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[28] THE GAS-DENSITY GRADIENT FOR 3 DARK INTERSTELLAR CLOUDS
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[30] INTERSTELLAR GAS AROUND WO STARS IN THE GALAXY AND THE MAGELLANIC CLOUDS
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