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Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength
Wang, Zhen; Chen, Xi; Gao, Feng; Zhang, Shaobo; Zheng, Xing-Wu; Ip, Wing-Huen; Wang, Na; Liu, Xiang; Zuo, Xiu-Ting; Gou, Wei; Chang, Sheng-Qi
2017
发表期刊ASTRONOMICAL JOURNAL
卷号154期号:6页码:249
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.
DOI10.3847/1538-3881/aa97db
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文献类型期刊论文
条目标识符http://libir.pmo.ac.cn/handle/332002/17896
专题期刊(老文献)
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Wang, Zhen,Chen, Xi,Gao, Feng,et al. Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength[J]. ASTRONOMICAL JOURNAL,2017,154(6):249.
APA Wang, Zhen.,Chen, Xi.,Gao, Feng.,Zhang, Shaobo.,Zheng, Xing-Wu.,...&Chang, Sheng-Qi.(2017).Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength.ASTRONOMICAL JOURNAL,154(6),249.
MLA Wang, Zhen,et al."Observations of the Hydroxyl Radical in C/2013 US10 (Catalina) at 18cm Wavelength".ASTRONOMICAL JOURNAL 154.6(2017):249.
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