A 1.3 cm line survey toward Orion KL
文献类型：期刊论文
| 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 |
| 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 |
| 学科主题 | 天文和天体物理 |
| 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 |
| 语种 | 英语 |
| WOS记录号 | WOS:000361803900048 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/14819]  |
| 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.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 |
| 推荐引用方式 GB/T 7714 | Gong, Y.,Henkel, C.,Thorwirth, S.,et al. A 1.3 cm line survey toward Orion KL[J]. ASTRONOMY & ASTROPHYSICS,2015,581:A48. |
| APA | Gong, Y..,Henkel, C..,Thorwirth, S..,Spezzano, S..,Menten, K. M..,...&Klein, B..(2015).A 1.3 cm line survey toward Orion KL.ASTRONOMY & ASTROPHYSICS,581,A48. |
| MLA | Gong, Y.,et al."A 1.3 cm line survey toward Orion KL".ASTRONOMY & ASTROPHYSICS 581(2015):A48. |
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来源：紫金山天文台
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