| pubmed-article:15846339 | rdf:type | pubmed:Citation | lld:pubmed |
| pubmed-article:15846339 | lifeskim:mentions | umls-concept:C0347997 | lld:lifeskim |
| pubmed-article:15846339 | pubmed:issue | 7036 | lld:pubmed |
| pubmed-article:15846339 | pubmed:dateCreated | 2005-4-22 | lld:pubmed |
| pubmed-article:15846339 | pubmed:abstractText | The birth of very massive stars is not well understood, in contrast to the formation process of low-mass stars like our Sun. 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. 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 has therefore generated considerable interest. Here we show that this protostar has an intermediate mass of only 2.5 to 8 solar masses (M(o), contrary to the earlier claim of 20M(o) (ref. 8). The surrounding circumstellar envelope contains only 0.09M(o) and a much more extended local molecular cloud has 4-9M(o). | lld:pubmed |
| pubmed-article:15846339 | pubmed:language | eng | lld:pubmed |
| pubmed-article:15846339 | pubmed:journal | http://linkedlifedata.com/r... | lld:pubmed |
| pubmed-article:15846339 | pubmed:status | PubMed-not-MEDLINE | lld:pubmed |
| pubmed-article:15846339 | pubmed:month | Apr | lld:pubmed |
| pubmed-article:15846339 | pubmed:issn | 1476-4687 | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:MiyataTakashi... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:TeradaHiroshi... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:OnakaTakashiT | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:YamashitaTaku... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:KatazaHirokaz... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:HondaMitsuhik... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:SakoShigeyuki... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:FujiyoshiTaku... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:OkamotoYoshik... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:KamazakiTakes... | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:JiangZhiboZ | lld:pubmed |
| pubmed-article:15846339 | pubmed:author | pubmed-author:HanawaTomoyuk... | lld:pubmed |
| pubmed-article:15846339 | pubmed:issnType | Electronic | lld:pubmed |
| pubmed-article:15846339 | pubmed:day | 21 | lld:pubmed |
| pubmed-article:15846339 | pubmed:volume | 434 | lld:pubmed |
| pubmed-article:15846339 | pubmed:owner | NLM | lld:pubmed |
| pubmed-article:15846339 | pubmed:authorsComplete | Y | lld:pubmed |
| pubmed-article:15846339 | pubmed:pagination | 995-8 | lld:pubmed |
| pubmed-article:15846339 | pubmed:year | 2005 | lld:pubmed |
| pubmed-article:15846339 | pubmed:articleTitle | No high-mass protostars in the silhouette young stellar object M17-SO1. | lld:pubmed |
| pubmed-article:15846339 | pubmed:affiliation | Department of Astronomy, School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan. sako@ioa.s.u-tokyo.ac.jp | lld:pubmed |
| pubmed-article:15846339 | pubmed:publicationType | Journal Article | lld:pubmed |
