ORION INFRARED NEBULA MOLECULAR CLOUD

被引：48

作者：

ZUCKERMAN, B

PALMER, P

机构：

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

[2] UNIV CALIF,BERKELEY,CA

[3] UNIV CHICAGO,DEPT ASTRON,1100 14 E 58TH ST,CHICAGO,IL 60637

来源：

关键词：

D O I：

10.1086/181843

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L35 / L38

页数：4

共 47 条

[21] NEW INTERSTELLAR METHANOL LINES
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[22] CO AND CS IN ORION NEBULA
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[23] MASER MODEL FOR INTERSTELLAR OH MICROWAVE EMISSION
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[26] 18-CM OBSERVATIONS OF GALACTIC OH FROM LONGITUDES 128 DEGREES TO 300 DEGREES
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[27] STRUCTURE OF OH SOURCE IN W3
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[J]. ASTROPHYSICAL JOURNAL, 1968, 152 (2P2) : L97 - &
[28] VERY LONG BASELINE INTERFEROMETRIC OBSERVATIONS OF H2O SOURCES IN W49 N,W3(OH), ORION A, AND VY CANIS MAJORIS
MORAN, JM
PAPADOPOULOS, GD
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[J]. ASTROPHYSICAL JOURNAL, 1973, 185 (02) : 535 - 567
[29] IRC+10216 MOLECULAR ENVELOPE
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[J]. ASTROPHYSICAL JOURNAL, 1975, 197 (03) : 603 - 610
[30] MORRIS M, TO BE PUBLISHED