CO emission toward HI absorption sources in the large magellanic cloud

被引:0
作者
Marx-Zimmer, M
Zimmer, F
Herbstmeier, U
Dickey, JM
机构
[1] Univ Bonn, Inst Radioastron, D-53121 Bonn, Germany
[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[3] Univ Minnesota, Dept Astron, Minneapolis, MN 55455 USA
来源
NEW VIEWS OF THE MAGELLANIC CLOUDS | 1999年 / 190期
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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页码:124 / 125
页数:2
相关论文
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[2]  
DESPOIS D, 1985, ASTRON ASTROPHYS, V148, P83
[3]  
DICKEY JM, 1994, ASTRON ASTROPHYS, V289, P357
[4]  
MARXZIMMER M, 1998, P WORKSH MAG CLOUDS, P275
[5]   H I clouds in the large magellanic cloud, cooler than in the galaxy? [J].
Mebold, U ;
Dusterberg, C ;
Dickey, JM ;
StaveleySmith, L ;
Kalberla, P .
ASTROPHYSICAL JOURNAL, 1997, 490 (01) :L65-L68