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PMO OpenIR  > 毫米波和亚毫米波技术实验室  > 期刊论文
题名: Massive Star Formation: Accreting from Companion
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
文章类型: Article
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
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/15738
Appears in Collections:毫米波和亚毫米波技术实验室_期刊论文

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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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