中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Massive Star Formation: Accreting from Companion

文献类型:期刊论文

作者Chen, X.1; Zhang, J. S.2
刊名JOURNAL OF ASTROPHYSICS AND ASTRONOMY
出版日期2014-09-01
卷号35期号:3页码:495-496
关键词Infrared: ISM stars: formation ISM: jets and outflows
英文摘要We report the possible accretion from companion in the massive star forming region (G350.69-0.49). This region seems to be a binary system composed of a diffuse object (possible nebulae or UC HII region) and a Massive Young Stellar Object (MYSO) seen in Spitzer IRAC image. The diffuse object and MYSO are connected by the shock-excited 4.5 mu m emission, suggesting that the massive star may form through accreting material from the companion in this system.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
收录类别SCI
语种英语
WOS记录号WOS:000350481700068
源URL[http://libir.pmo.ac.cn/handle/332002/15748]  
专题紫金山天文台_毫米波和亚毫米波技术实验室
作者单位1.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Radio Astron, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
2.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China
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GB/T 7714
Chen, X.,Zhang, J. S.. Massive Star Formation: Accreting from Companion[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2014,35(3):495-496.
APA Chen, X.,&Zhang, J. S..(2014).Massive Star Formation: Accreting from Companion.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,35(3),495-496.
MLA Chen, X.,et al."Massive Star Formation: Accreting from Companion".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 35.3(2014):495-496.

入库方式: OAI收割

来源:紫金山天文台

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