中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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; Menten, K. M.2; Goldsmith, P. F.5
刊名ASTRONOMY & ASTROPHYSICS
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
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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.

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来源:紫金山天文台

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