WARM NEUTRAL HALOS AROUND MOLECULAR CLOUDS .2. H-I AND CO (J = 1-0) OBSERVATIONS

被引:29
作者
WANNIER, PG
ANDERSSON, BG
MORRIS, M
LICHTEN, SM
机构
[1] GOTHENBURG UNIV,S-41124 GOTHENBURG,SWEDEN
[2] UNIV CALIF LOS ANGELES,DEPT ASTRON,LOS ANGELES,CA 90024
关键词
INTERSTELLAR; MOLECULES; RADIO SOURCES; 21-CM RADIATION;
D O I
10.1086/191557
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observational data are presented relating to the boundary regions between dense, molecular clouds and the more diffuse atomic gas. The data set consists of H I 21 cm and CO (J = 1-0) strip maps in 14 molecule clouds which traverse 62 known CO cloud boundaries. The angular lengths of the strips range from 0.5-degrees to several degrees of arc, which is generally adequate to eliminate confusion with background (and foreground) H I. Most of the crossed boundaries (49 of 62) show clear evidence for the presence of H I emission maxima, or halos, lying outside the molecular clouds' gas. There is also general evidence for limb brightening in the CO emission.
引用
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页码:987 / 998
页数:12
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