PMO OpenIR  > 毫米波和亚毫米波技术实验室
Massive Star Formation: Accreting from Companion
Chen, X.1; Zhang, J. S.2
2014-09-01
Source PublicationJOURNAL OF ASTROPHYSICS AND ASTRONOMY
Volume35Issue:3Pages:495-496
AbstractWe 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.
KeywordInfrared: Ism Stars: Formation Ism: Jets And Outflows
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000350481700068
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/15748
Collection毫米波和亚毫米波技术实验室
Affiliation1.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
Recommended Citation
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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