High-mass Outflows Identified from COHRS CO (3-2) Survey
文献类型:期刊论文
作者 | Baan, W. A.2,3; He, Yuxin2,6; Zhexeray, Dauren4; Ji, Weiguang2,6; Tang, Xindi2,5,6; Wu, Gang2,6; Esimbek, Jarken2,6; Li, Dalei2,6; Zhou, Jianjun2,6; Li, Qiang1,2 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2018-11-10 |
卷号 | 867期号:2页码:167 |
ISSN号 | 0004-637X |
关键词 | ISM: jets and outflows ISM: molecules stars: formation stars: massive |
DOI | 10.3847/1538-4357/aae2b8 |
产权排序 | 1 |
英文摘要 | An unbiased search of molecular outflows within the region of the CO High Resolution survey has identified 157 high-mass outflows from a sample of 770 APEX Telescope Large Area Survey of the Galaxy clumps with a detection rate of 20%. The detection rate of outflows increases for clumps with higher M-clump, L-bol, L-bol/M-clump, N-H2, and T-dust compared to the clumps with no outflow. The detection rates of the outflow increase from protostellar (8%) to young stellar object clump (17%) to massive star-forming clump (29%). The detection rate 26% for quiescent clump is preliminary, because the sample of quiescent clumps is small. A statistical relation between the outflow and clump masses for our sample is log(M-out/M-circle dot) = (-1.1 +/- 0.21) + (0.9 +/- 0.07) log(M-clump/M-circle dot). The detection rate of outflows and the outflow mass-loss rate show an increase with increasing M-clump,M- L-bol, N-H2, and T-dust, which indicates that clumps with outflow with higher parameter values are at a more advanced evolutionary stage. The outflow mechanical force increases with increasing bolometric luminosities. No clear evidence has yet been found that highermass outflows have different launching conditions than low-mass outflows. |
WOS关键词 | BIPOLAR MOLECULAR OUTFLOWS ; STAR-FORMATION REGIONS ; YOUNG STELLAR OBJECTS ; PROTOSTELLAR CANDIDATES ; FORMING REGIONS ; LINE EMISSION ; SAMPLE ; EVOLUTION ; FREQUENCY ; ATLASGAL |
资助项目 | National Natural Science foundation of China[11373062] ; National Natural Science Foundation of China[11433008] ; National Natural Science Foundation of China[11703073] ; National Natural Science Foundation of China[11703074] ; National Natural Science Foundation of China[11603063] ; Program of the Light in China's Western Region (LCRW)[2016-QNXZ-B-22] ; Program of the Light in China's Western Region (LCRW)[2016-QNXZ-B-23] ; High-end Foreign Experts of the State Administration of Foreign Experts Affairs (SAFEA) of China[20176500001] ; High-end Foreign Experts of the State Administration of Foreign Experts Affairs (SAFEA) of China[20166500004] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000450221700034 |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/2244] |
专题 | 恒星形成与演化研究团组 |
通讯作者 | Li, Qiang |
作者单位 | 1.Univ Chinese Acad Sci, Beijing 100080, Peoples R China 2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 3.Netherlands Inst Radio Astron, NL-7991 PD Dwingeloo, Netherlands 4.AL Farabi Kazakh Natl Univ, Dept Solid State Phys & Nonlinear Phys, Fac Phys & Technol, Alma Ata 050040, Kazakhstan 5.Max Planck Inst Radioastron, D-53121 Bonn, Germany 6.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Peoples R China |
推荐引用方式 GB/T 7714 | Baan, W. A.,He, Yuxin,Zhexeray, Dauren,et al. High-mass Outflows Identified from COHRS CO (3-2) Survey[J]. ASTROPHYSICAL JOURNAL,2018,867(2):167. |
APA | Baan, W. A..,He, Yuxin.,Zhexeray, Dauren.,Ji, Weiguang.,Tang, Xindi.,...&Li, Qiang.(2018).High-mass Outflows Identified from COHRS CO (3-2) Survey.ASTROPHYSICAL JOURNAL,867(2),167. |
MLA | Baan, W. A.,et al."High-mass Outflows Identified from COHRS CO (3-2) Survey".ASTROPHYSICAL JOURNAL 867.2(2018):167. |
入库方式: OAI收割
来源:新疆天文台
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