中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
SUBARCSECOND OBSERVATIONS OF NGC 7538 IRS 1: CONTINUUM DISTRIBUTION AND DYNAMICS OF MOLECULAR GAS

文献类型:期刊论文

作者Zhu, Lei1,2,3; Zhao, Jun-Hui2; Wright, M. C. H.4; Sandell, Goeran5; Shi, Hui1,6; Wu, Yue-Fang3; Brogan, Crystal7; Corder, Stuartt7
刊名ASTROPHYSICAL JOURNAL
出版日期2013-12-10
卷号779期号:1
关键词H II regions ISM: jets and outflows ISM: kinematics and dynamics ISM: molecules radio lines: ISM stars: formation
英文摘要We report new results based on the analysis of the Submillimeter Array (SMA) and Combined Array for Research in Millimeter-wave Astronomy (CARMA) observations of NGC 7538 IRS 1 at 1.3 and 3.4 mm with subarcsecond resolutions. With angular resolutions similar to 0.'' 7, the SMA and CARMA observations show that the continuum emission at 1.3 and 3.4 mm from the hyper-compact H II region IRS 1 is dominated by a compact source with a tail-like extended structure to the southwest of IRS 1. With a CARMA B-array image at 1.3 mm convolved to 0.'' 1, we resolve the hyper-compact H II region into two components: an unresolved hyper-compact core, and a north-south extension with linear sizes of <270 AU and similar to 2000 AU, respectively. The fine structure observed with CARMA is in good agreement with the previous Very Large Array results at centimeter wavelengths, suggesting that the hyper-compact H II region at the center of IRS 1 is associated with an ionized bipolar outflow. We image the molecular lines OCS(19-18) and CH3CN(12-11) as well as (CO)-C-13(2-1) surrounding IRS 1, showing a velocity gradient along the southwest-northeast direction. The spectral line profiles in (CO)-C-13(2-1), CO(2-1), and HCN(1-0) observed toward IRS 1 show broad redshifted absorption, providing evidence for gas infall with rates in the range of 3-10 x 10(-3) M-circle dot yr(-1) inferred from our observations.
收录类别SCI
语种英语
WOS记录号WOS:000328160100051
源URL[http://ir.bao.ac.cn/handle/114a11/6040]  
专题国家天文台_射电天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
3.Peking Univ, Dept Astron, Beijing 100871, Peoples R China
4.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
5.NASA, Ames Res Ctr, SOFIA USRA, Moffett Field, CA 94035 USA
6.Max Planck Inst Radioastron, D-53121 Bonn, Germany
7.NRAO, Charlottesville, VA 22903 USA
推荐引用方式
GB/T 7714
Zhu, Lei,Zhao, Jun-Hui,Wright, M. C. H.,et al. SUBARCSECOND OBSERVATIONS OF NGC 7538 IRS 1: CONTINUUM DISTRIBUTION AND DYNAMICS OF MOLECULAR GAS[J]. ASTROPHYSICAL JOURNAL,2013,779(1).
APA Zhu, Lei.,Zhao, Jun-Hui.,Wright, M. C. H..,Sandell, Goeran.,Shi, Hui.,...&Corder, Stuartt.(2013).SUBARCSECOND OBSERVATIONS OF NGC 7538 IRS 1: CONTINUUM DISTRIBUTION AND DYNAMICS OF MOLECULAR GAS.ASTROPHYSICAL JOURNAL,779(1).
MLA Zhu, Lei,et al."SUBARCSECOND OBSERVATIONS OF NGC 7538 IRS 1: CONTINUUM DISTRIBUTION AND DYNAMICS OF MOLECULAR GAS".ASTROPHYSICAL JOURNAL 779.1(2013).

入库方式: OAI收割

来源:国家天文台

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