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PMO OpenIR  > 分子云与恒星形成研究团组  > 期刊论文
题名: A 1.3 cm line survey toward Orion KL
作者: Gong, Y.1, 2, 4; Henkel, C.3, 5, 6; Thorwirth, S.; Spezzano, S.; Menten, K. M.3; Walmsley, C. M.7, 8; Wyrowski, F.3; Mao, R. Q.1, 2; Klein, B.3, 9
刊名: ASTRONOMY & ASTROPHYSICS
出版日期: 2015-09-01
卷号: 581, 页码:A48
关键词: astrochemistry ; ISM: individual objects: Orion KL ; ISM: molecules ; radio lines: ISM ; surveys
学科分类: 天文和天体物理
DOI: 10.1051/0004-6361/201526275
文章类型: Article
英文摘要: Context. The nearby Orion Kleinmann-Low nebula is one of the most prolific sources of molecular line emission. It has served as a benchmark for spectral line searches throughout the (sub) millimeter regime.
WOS标题词: Science & Technology ; Physical Sciences
类目[WOS]: Astronomy & Astrophysics
研究领域[WOS]: Astronomy & Astrophysics
关键词[WOS]: MILLIMETER-WAVE OBSERVATIONS ; RADIO RECOMBINATION LINES ; GHZ SPECTRAL SURVEY ; H-II REGIONS ; HELIUM ABUNDANCE ; HOT CORE ; PHYSICAL CONDITIONS ; MOLECULAR CLOUD ; KLEINMANN-LOW ; INTERSTELLAR-MOLECULES
收录类别: SCI
所属项目名称: PMO_LIB-IR
语种: 英语
WOS记录号: WOS:000361803900048
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/14819
Appears in Collections:分子云与恒星形成研究团组_期刊论文

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作者单位: 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China
3.Max Planck Inst Radioastron, D-53121 Bonn, Germany
4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
5.King Abdulaziz Univ, Dept Astron, Jeddah 21589, Saudi Arabia
6.Univ Cologne, Phys Inst 1, D-50937 Cologne, Germany
7.Osserv Astrofis Arcetri, I-50125 Florence, Italy
8.Dublin Inst Adv Studies, Dublin 2, Ireland
9.Univ Appl Sci Bonn Rhein Sieg, D-53757 St Augustin, Germany
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