THE (J,K) = (3,3) INVERSION LINE OF NH3 - A POSSIBLE INTERSTELLAR CHRONOMETER

被引：0

作者：

FLOWER, DR ^{[1
]}

OFFER, A ^{[1
]}

SCHILKE, P ^{[1
]}

机构：

[1] MAX PLANCK INST RADIOASTRON,W-5300 BONN 1,GERMANY

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D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：P4 / P8

页数：5

共 18 条

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[2] ROTATIONAL-EXCITATION OF ORTHO-NH3 BY PARA-H-2
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FLOWER, DR
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[3] ROTATIONAL-EXCITATION OF PARA-NH3 BY PARA-H-2
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[J]. JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS, 1987, 20 (05) : 1039 - 1058
[4] DESFORETS GP, 1990, IN PRESS MON NOT R A
[5] ON THE ORTHO-H-2 PARA-H-2 RATIO IN MOLECULAR CLOUDS
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[6] GUILLOTEAU S, 1983, ASTRON ASTROPHYS, V124, P322
[7] VLA OBSERVATIONS OF THE (NH3)-N-15 MASER ASSOCIATED WITH NGC-7538 IRS-1
JOHNSTON, KJ
STOLOVY, SR
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[J]. ASTROPHYSICAL JOURNAL, 1989, 343 (02) : L41 - L44
[8] NEW INTERSTELLAR MASERS IN NONMETASTABLE AMMONIA
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[J]. ASTROPHYSICAL JOURNAL, 1986, 300 (02) : L79 - L84
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[10] MAUERSBERGER R, 1987, ASTRON ASTROPHYS, V173, P352