Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength

doi:10.3847/1538-3881/aa97db

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	Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength
	Zhang, Shaobo 2; Chang, Sheng-Qi 6; Gou, Wei 6; Zuo, Xiu-Ting 6; Liu, Xiang1 ; Wang, Na1 ; Ip, Wing-Huen 4,5; Zheng, Xing-Wu 3; Gao, Feng 6; Chen, Xi 6
刊名	ASTRONOMICAL JOURNAL
	2017-12-01
卷号	154 期号:6 页码:249
关键词	Comets: General Line: Profiles Molecular Processes
ISSN号	0004-6256
DOI	10.3847/1538-3881/aa97db
产权排序	1
文献子类	Article
英文摘要	The hydroxyl (OH) radical produced by photodissociation of water molecule is one of the most important indicators for cometary outgassing activity. The absorption lines of the OH radical at 1665 and 1667 MHz in the coma of comet C/2013 US10 Catalina were detected between 2015 December 3 and 5 by the Tian Ma Radio Telescope of Shanghai Astronomical Observatory. The source flux intensity was derived to be about - 209 mJy km s(-1) and -86 mJy km s(-1) at 1665 MHz and 1667 MHz, respectively. The corresponding gas production rate was estimated to be (8.78 +/- 1.47) x 10(28) H2O s(-1) and (5.94 +/- 1.27) x 10(28) H2O s(-1), accordingly.
URL标识	查看原文
WOS关键词	Comet-west 1975n ; Oh Line-shapes ; O1 Hale-bopp ; Molecular-spectroscopy ; Microwave Transitions ; Expansion Velocity ; Cologne Database ; Emission ; Halley ; P/halley
WOS研究方向	Astronomy & Astrophysics
语种	英语
WOS记录号	WOS:000416028700002
资助机构	National Nature Science Foundation of China (grant NSFC)(11503073) ; Chinese Academy of Sciences Foundation of the young scholars of western(2015-XBQN-B-02) ; Ministry of Science and Technology of Taiwan(MOST 104-2119-M-008-024, NSC 102-2112-M-008-013-MY3, MOST 104-2111-M-008-020) ; FDCT grant of Macau Special Administrative Region(017/2014/A1, 039/2013/A2)
内容类型	期刊论文
源URL	[http://ir.xao.ac.cn/handle/45760611-7/1934]
专题	星系宇宙学研究团组新疆天文台_射电天文研究室新疆天文台_其它新疆天文台_110米口径全可动射电望远镜（SmART）_110米大口径全可动射电望远镜关键技术研究（973项目）_课题1：大样本射电天体的观测和前沿问题研究
通讯作者	Wang, Zhen
作者单位	1.Key Laboratory of Radio Astronomy, Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, Xinjiang 830011, China 2.Purple Mountain Observatory, and Key Laboratory for Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China 3.Astronomy Department, Nanjing University, Nanjing 210093, China 4.Institute of Astronomy, National Center University, Taiwan 5.Space Science Institute, Macau University of Science and Technology, Macau 6.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
推荐引用方式 GB/T 7714	Zhang, Shaobo,Chang, Sheng-Qi,Gou, Wei,et al. Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength[J]. ASTRONOMICAL JOURNAL,2017,154(6):249.
APA	Zhang, Shaobo.,Chang, Sheng-Qi.,Gou, Wei.,Zuo, Xiu-Ting.,Liu, Xiang.,...&Wang, Zhen.(2017).Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength.ASTRONOMICAL JOURNAL,154(6),249.
MLA	Zhang, Shaobo,et al."Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength".ASTRONOMICAL JOURNAL 154.6(2017):249.