EVIDENCE FOR INTERSTELLAR H2O IN THE ORION MOLECULAR CLOUD

被引：16

作者：

KNACKE, RF ^{[1
]}

LARSON, HP ^{[1
]}

NOLL, KS ^{[1
]}

机构：

[1] UNIV ARIZONA, LUNAR & PLANETARY LAB, TUCSON, AZ 85721 USA

来源：

ASTROPHYSICAL JOURNAL | 1988年 / 335卷 / 01期

关键词：

D O I：

10.1086/185332

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L27 / L30

页数：4

共 16 条

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[3] INFRARED FOURIER SPECTROMETER FOR AIRBORNE AND GROUND-BASED ASTRONOMY [J].

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LARSON, HP ;

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MICHEL, G ;

CONNES, P .

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[4]

Gates D. M., 1964, NBS MONOGRAPH, V71

[5]

HOUCK JR, 1974, AP J, V193, P139

[6]

IRVINE WM, 1988, IN PRESS ORIGIN EVOL

[7]

JONG TD, 1973, ASTRON ASTROPHYS, V26, P297

[8] SEARCH FOR INTERSTELLAR METHANE [J].

KNACKE, RF ;

GEBALLE, TR ;

NOLL, KS ;

TOKUNAGA, AT .

ASTROPHYSICAL JOURNAL, 1985, 298 (02) :L67-L69

[9]

LARSON HP, 1989, IN PRESS AP J

[10] SYNTHESIS OF COMPLEX-MOLECULES IN DENSE INTERSTELLAR CLOUDS VIA GAS-PHASE CHEMISTRY - A PSEUDO TIME-DEPENDENT CALCULATION [J].

LEUNG, CM ;

HERBST, E ;

HUEBNER, WF .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1984, 56 (02) :231-256

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