Spectral energy distributions of 6.7 GHz methanol masers
文献类型:期刊论文
作者 | Pandian, J. D.1,2; Momjian, E.3; Xu, Y.4![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2010-11-01 |
卷号 | 522页码:A8 |
关键词 | masers stars: formation HII regions |
ISSN号 | 0004-6361 |
英文摘要 | Context. The 6.7 GHz maser transition of methanol has been found exclusively towards massive star forming regions. A majority of the masers have been found to lack the presence of any associated radio continuum. This could be due to the maser emission originating prior to the formation of an HII region around the central star, or from the central object being too cool to produce a HII region. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | RADIO-CONTINUUM EMISSION ; ULTRACOMPACT HII-REGIONS ; YOUNG STELLAR OBJECTS ; GALACTIC PLANE SURVEY ; STAR-FORMING REGIONS ; HIGH-MASS PROTOSTARS ; H II REGIONS ; VLBI OBSERVATIONS ; HIGH-RESOLUTION ; MU-M |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000284153100014 |
公开日期 | 2011-11-23 |
源URL | [http://159.226.72.40/handle/332002/1219] ![]() |
专题 | 紫金山天文台_紫金山天文台青海观测站 |
作者单位 | 1.Univ Hawaii, Inst Astron, Honolulu, HI 96814 USA 2.Max Planck Inst Radioastron, D-53121 Bonn, Germany 3.Natl Radio Astron Observ, Socorro, NM 87801 USA 4.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 5.CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA |
推荐引用方式 GB/T 7714 | Pandian, J. D.,Momjian, E.,Xu, Y.,et al. Spectral energy distributions of 6.7 GHz methanol masers[J]. ASTRONOMY & ASTROPHYSICS,2010,522:A8. |
APA | Pandian, J. D.,Momjian, E.,Xu, Y.,Menten, K. M.,&Goldsmith, P. F..(2010).Spectral energy distributions of 6.7 GHz methanol masers.ASTRONOMY & ASTROPHYSICS,522,A8. |
MLA | Pandian, J. D.,et al."Spectral energy distributions of 6.7 GHz methanol masers".ASTRONOMY & ASTROPHYSICS 522(2010):A8. |
入库方式: OAI收割
来源:紫金山天文台
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