中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
No high-mass protostars in the silhouette young stellar object M17-S01

文献类型:期刊论文

作者Sako, S; Yamashita, T; Kataza, H; Miyata, T; Okamoto, YK; Honda, M; Fujiyoshi, T; Terada, H; Kamazaki, T; Jiang, ZB
刊名NATURE
出版日期2005-04-21
卷号434期号:7036页码:995-998
关键词MOLECULAR CLOUD SUBARU TELESCOPE HIGH-RESOLUTION CO EMISSION STARS M17 REGION ENVELOPES ROTATION CAMERA
ISSN号0028-0836
英文摘要The birth of very massive stars is not well understood(1-3), in contrast to the formation process of low-mass stars like our Sun(4,5). It is not even clear that massive stars can form as single entities; rather, they might form through the mergers of smaller ones born in tight groups(6,7). The recent claim of the discovery of a massive protostar in M17 (a nearby giant ionized region) forming through the same mechanism as low-mass stars(8) has therefore generated considerable interest. Here we show that this protostar has an intermediate mass of only 2.5 to 8 solar masses (M.), contrary to the earlier claim of 20. (ref. 8). The surrounding circumstellar envelope contains only 0.09M. and a much more extended local molecular cloud has 4-9M..
WOS标题词Science & Technology
学科主题Astronomy & Astrophysics
类目[WOS]Multidisciplinary Sciences
研究领域[WOS]Science & Technology - Other Topics
关键词[WOS]MOLECULAR CLOUD ; SUBARU TELESCOPE ; HIGH-RESOLUTION ; CO EMISSION ; STARS ; M17 ; REGION ; ENVELOPES ; ROTATION ; CAMERA
收录类别SCI
语种英语
WOS记录号WOS:000228524600031
公开日期2012-03-07
源URL[http://159.226.72.40/handle/332002/4054]  
专题紫金山天文台_分子云与恒星形成研究团组
作者单位1.Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
2.Natl Inst Nat Sci, Natl Astron Observ Japan, Subaru Telescope, Hilo, HI 96720 USA
3.Univ Tokyo, Inst Astron, Tokyo 1810015, Japan
4.Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Kanagawa 2298510, Japan
5.Ibaraki Univ, Inst Astrophys & Planetary Sci, Mito, Ibaraki 3108512, Japan
6.Chinese Acad Sci, Natl Astron Observ, Purple Mt Observ, Nanjing 210008, Peoples R China
7.Chiba Univ, Ctr Fontier Sci, Inage Ku, Chiba 2638522, Japan
推荐引用方式
GB/T 7714
Sako, S,Yamashita, T,Kataza, H,et al. No high-mass protostars in the silhouette young stellar object M17-S01[J]. NATURE,2005,434(7036):995-998.
APA Sako, S.,Yamashita, T.,Kataza, H.,Miyata, T.,Okamoto, YK.,...&Onaka, T.(2005).No high-mass protostars in the silhouette young stellar object M17-S01.NATURE,434(7036),995-998.
MLA Sako, S,et al."No high-mass protostars in the silhouette young stellar object M17-S01".NATURE 434.7036(2005):995-998.

入库方式: OAI收割

来源:紫金山天文台

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