POSSIBLE RELATION BETWEEN AN OH SOURCE AND AN INFRARED OBJECT IN ORION NEBULA

被引：47

作者：

RAIMOND, E

ELIASSON, B

机构：

来源：

ASTROPHYSICAL JOURNAL | 1967年 / 150卷 / 3P2期

关键词：

D O I：

10.1086/180118

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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页码：L171 / &

相关论文

共 5 条

[1] OBSERVATIONS OF AN INFRARED STAR IN ORION NEBULA
BECKLIN, EE
NEUGEBAUER, G
[J]. ASTROPHYSICAL JOURNAL, 1967, 147 (02) : 799 - +
[2] DISCOVERY OF AN INFRARED NEBULA IN ORION
KLEINMAN.DE
LOW, FJ
[J]. ASTROPHYSICAL JOURNAL, 1967, 149 (1P2) : L1 - &
[3] SPECTRAL LINE INTERFEROMETRY WITH INDEPENDENT TIME STANDARDS AT STATIONS SEPARATED BY 845 KILOMETERS
MORAN, JM
CROWTHER, PP
BURKE, BF
BARRETT, AH
ROGERS, AEE
BALL, JA
CARTER, JC
BARE, CC
[J]. SCIENCE, 1967, 157 (3789) : 676 - &
[4] OBSERVATIONS OF GALACTIC OH
PALMER, P
ZUCKERMAN, B
[J]. ASTROPHYSICAL JOURNAL, 1967, 148 (3P1) : 727 - +
[5] SOLOMON PM, IN PRESS