MOLECULAR LINES OF 13 GALACTIC INFRARED BUBBLE REGIONS
文献类型：期刊论文
| 作者 | Yan,Qing-zeng1,2,3; Xu,Ye1; Zhang,Bo2; Lu,Deng-rong1; Chen,Xi2; Tang,Zheng-hong2 |
| 刊名 | The Astronomical Journal
 |
| 出版日期 | 2016-10-14 |
| 卷号 | 152期号:5 |
| ISSN号 | 0004-6256 |
| 关键词 | ISM: bubbles ISM: clouds ISM: jets and outflows ISM: kinematics and dynamics ISM: molecules stars: formation |
| DOI | 10.3847/0004-6256/152/5/117 |
| 英文摘要 | ABSTRACT We investigated the physical properties of molecular clouds and star formation (SF) processes around infrared bubbles, which are essentially expanding H ii regions. We performed observations of 13 galactic infrared bubble fields containing 18 bubbles. We observed five molecular lines—12CO ( ), 13CO ( ), C18O ( ), HCN ( ), and HCO+ ( )—and several publicly available surveys were used for comparison: Galactic Legacy Infrared Mid-Plane Survey Extraordinaire, Multiband Imaging Photometer for Spitzer Galactic Plane Survey, APEX Telescope Large Area Survey of the Galaxy, Bolocam Galactic Plane Survey, Very Large Array (VLA) Galactic Plane Survey, Multi-Array Galactic Plane Imaging Survey, and NRAO VLA Sky Survey. We find that these bubbles are generally connected with molecular clouds, most of which are giant. Several bubble regions display velocity gradients and broad-shifted profiles, which could be due to the expansion of bubbles. The masses of molecular clouds within bubbles range from 100 to 19,000 M⊙, and their dynamic ages are about 0.3–3.7 Myr, which takes into account the internal turbulence pressure of surrounding molecular clouds. Clumps are found in the vicinity of all 18 bubbles, and molecular clouds near four of these bubbles with larger angular sizes show shell-like morphologies, indicating that either collect-and-collapse or radiation-driven implosion processes may have occurred. Due to the contamination of adjacent molecular clouds, only six bubble regions are appropriate to search for outflows, and we find that four have outflow activities. Three bubbles display ultra-compact H ii regions at their borders, and one is probably responsible for its outflow. In total, only six bubbles show SF activities in the vicinity, and we suggest that SF processes might have been triggered. |
| 语种 | 英语 |
| 出版者 | The American Astronomical Society |
| WOS记录号 | IOP:0004-6256-152-5-117 |
| 源URL | [http://119.78.226.72/handle/331011/32157]  |
| 专题 | 中国科学院上海天文台 |
| 作者单位 | 1.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China; xuye@pmo.ac.cn 2.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China; qzyan@shao.ac.cn 3.International Center for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth WA 6845, Australia |
| 推荐引用方式 GB/T 7714 | Yan,Qing-zeng,Xu,Ye,Zhang,Bo,et al. MOLECULAR LINES OF 13 GALACTIC INFRARED BUBBLE REGIONS[J]. The Astronomical Journal,2016,152(5). |
| APA | Yan,Qing-zeng,Xu,Ye,Zhang,Bo,Lu,Deng-rong,Chen,Xi,&Tang,Zheng-hong.(2016).MOLECULAR LINES OF 13 GALACTIC INFRARED BUBBLE REGIONS.The Astronomical Journal,152(5). |
| MLA | Yan,Qing-zeng,et al."MOLECULAR LINES OF 13 GALACTIC INFRARED BUBBLE REGIONS".The Astronomical Journal 152.5(2016). |
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来源：上海天文台
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