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
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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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