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Massive Star Formation: Accreting from Companion
Chen, X.1; Zhang, J. S.2
2014-09-01
发表期刊JOURNAL OF ASTROPHYSICS AND ASTRONOMY
卷号35期号:3页码:495-496
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.
文章类型Article
关键词Infrared: Ism Stars: Formation Ism: Jets And Outflows
WOS标题词Science & Technology ; Physical Sciences
收录类别SCI
语种英语
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000350481700068
引用统计
文献类型期刊论文
条目标识符http://libir.pmo.ac.cn/handle/332002/15748
专题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.
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