WHY C-12 O-16 PROFILES IN DARK CLOUDS DO NOT HAVE FLAT TOPS

被引：6

作者：

MILMAN, AS ^{[1
]}

机构：

[1] UNIV MARYLAND,ASTRON PROGRAM,COLLEGE PK,MD 20742

来源：

ASTROPHYSICAL JOURNAL | 1974年 / 193卷 / 02期

关键词：

D O I：

10.1086/181640

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L93 / L96

页数：4

共 8 条

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[3]

Lynds B. T., 1962, ApJS, V7, P1, DOI [DOI 10.1086/190072, 10.1086/190072]

[4]

MILMAN AS, 1973, B AM ASTRON SOC, V5, P332

[5]

MILMAN AS, IN PRESS

[6] C-133-16-C-12-O-18 RATIOS IN 9 H II REGIONS [J].

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SOLOMON, PM ;

WILSON, RW ;

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JEFFERTS, KB .

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[7] CARBON-MONOXIDE OBSERVATIONS OF DENSE INTERSTELLAR CLOUDS [J].

PENZIAS, AA ;

SOLOMON, PM ;

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JEFFERTS, KB .

ASTROPHYSICAL JOURNAL, 1972, 174 (01) :L43-&

[8] RADIATIVE-TRANSFER, EXCITATION, AND COOLING OF MOLECULAR EMISSION-LINES (CO AND CS) [J].

SCOVILLE, NZ ;

SOLOMON, PM .

ASTROPHYSICAL JOURNAL, 1974, 187 (02) :L67-L71

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