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 |
推荐引用方式 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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