Hidden Star Formation in High-Velocity Gas Clouds in Clump 2 near the Edge of the CMZ

被引:0
|
作者
Tolls, Volker [1 ]
Smith, Howard A. [1 ]
机构
[1] Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02478 USA
来源
关键词
Galaxy: center; Galaxy: kinematics and dynamics; Galaxy: structure; ISM: clouds; ISM: kinematics and dynamics; stars: formation; GALACTIC-CENTER;
D O I
10.1017/S1743921316012199
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a snapshot of our ongoing investigation of molecular clouds in Clump 2 located in the Galactic Bar region at a projected distance of similar to 400pc from the Galactic Center. We show that the analysis of the Clump 2 molecular clouds is complicated because of many fore- and background clouds in the line of sight. Of all clouds, IGGC 22 is the most interesting one, showing very high dust column densities, significant high-J CO emission, and, potentially harbors star formations as eluded to by the detection of [OIII] emission.
引用
收藏
页码:170 / 171
页数:2
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