KMS National Astronomical Observatories, CAS
Molecular outflows and gas rotation associated with G20.08-0.14N | |
Yu NaiPing1; Wang JunJie1 | |
2013 | |
Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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ISSN | 1674-4527 |
Volume | 13Issue:11Pages:1295 |
Abstract | We present the results of a high-resolution study with the Submillimeter Array (SMA) toward the massive star-forming complex G20.08-0.14N. With the SMA data, we have detected and analyzed the transitions in the (CO)-C-12 (3-2) and (CO)-C-12 (2-1) molecular lines as well as CH3CN. The millimeter observations reveal highly collimated bipolar molecular outflows, traced by high-velocity (CO)-C-12 (2-1) and (CO)-C-12 (3-2) emissions. Using a rotation temperature diagram, we derive that the rotational temperature and the column density of CH3CN are 244 K and 1.2x10(15) cm(-2), respectively. We also suggest that the minor outflow is probably driven by the hypercompact (HC) HII region A that is inside. We find the molecular gas (traced by (CO)-O-17, SO, CH3OH and SO2) surrounding G20.08-0.14N appears to be undergoing bulk rotation. The HCHII region A that is inside is most probably the main source of accretion and heating for G20.08-0.14N. |
Keyword | MASSIVE STAR-FORMATION CO LINE FORMATION H-II REGIONS HII-REGIONS DYNAMICAL COLLAPSE BIPOLAR FLOWS RESOLUTION CORES G19.61-0.23 SAMPLE ISM: individual objects (G20.08-0.14N) ISM: molecules radio lines: ISM stars: formation ISM: kinematics and dynamics |
Language | 英语 |
Document Type | 期刊论文 |
Identifier | http://ir.bao.ac.cn/handle/114a11/63282 |
Collection | 中国科学院国家天文台 |
Affiliation | 1.中国科学院 2.中国科学院国家天文台 |
Recommended Citation GB/T 7714 | Yu NaiPing,Wang JunJie. Molecular outflows and gas rotation associated with G20.08-0.14N[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2013,13(11):1295. |
APA | Yu NaiPing,&Wang JunJie.(2013).Molecular outflows and gas rotation associated with G20.08-0.14N.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,13(11),1295. |
MLA | Yu NaiPing,et al."Molecular outflows and gas rotation associated with G20.08-0.14N".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 13.11(2013):1295. |
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