The Kinematic Distances of SNR G16.7+0.1 and G15.9+0.2 by Analyzing H i Absorption Spectra
文献类型：期刊论文
| 作者 | Tian,W. W.1,2,3; Zhu,H.1; Zhang,M. F.1,2; Chang,H. K.4,5; Shan,S. S.1,2; Leahy,D. A.3 |
| 刊名 | Publications of the Astronomical Society of the Pacific
 |
| 出版日期 | 2019-09-19 |
| 卷号 | 131期号:1005 |
| 关键词 | ISM: individual objects (SNR G16.7+0.1, G15.9+0.2) ISM: supernova remnants |
| ISSN号 | 0004-6280 |
| DOI | 10.1088/1538-3873/ab35f4 |
| 英文摘要 | Abstract We build H i absorption spectra toward Supernova Remnant (SNRs) G16.7+0.1 and G15.9+0.2 using the THOR survey data. With the absorption spectra, we give a new distance range of 7–16 kpc for G15.9+0.2. We also resolve the near/far-side distance ambiguity of G16.7+0.1 and confirm its kinematic distance of about 14 kpc. In addition, we analyze the CO (J?=?3–2) spectra toward G16.7+0.1 and find obvious CO emission at the 20 km s?1 OH 1720 MHz maser site. This supports Reynoso & Mangum suggestions that the velocity difference between the maser and southern molecular cloud is caused by the shock acceleration. We discuss the impact of the distances on other physical parameters of the two SNRs. |
| 语种 | 英语 |
| WOS记录号 | IOP:0004-6280-131-1005-AB35F4 |
| 出版者 | The Astronomical Society of the Pacific |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/27862]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 1.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China tww@bao.ac.cn, zhuhui@bao.ac.cn 2.University of Chinese Academy of Sciences, 19A Yuquan Road, Shijingshan District, Beijing 100049, People’s Republic of China 3.Department of Physics & Astronomy, University of Calgary, Calgary, Alberta T2N 1N4, Canada 4.Institute of Astronomy, National Tsing Hua University, Hsinchu 30013, Taiwan 5.Department of Physics, National Tsing Hua University, Hsinchu 30013, Taiwan |
| 推荐引用方式 GB/T 7714 | Tian,W. W.,Zhu,H.,Zhang,M. F.,et al. The Kinematic Distances of SNR G16.7+0.1 and G15.9+0.2 by Analyzing H i Absorption Spectra[J]. Publications of the Astronomical Society of the Pacific,2019,131(1005). |
| APA | Tian,W. W.,Zhu,H.,Zhang,M. F.,Chang,H. K.,Shan,S. S.,&Leahy,D. A..(2019).The Kinematic Distances of SNR G16.7+0.1 and G15.9+0.2 by Analyzing H i Absorption Spectra.Publications of the Astronomical Society of the Pacific,131(1005). |
| MLA | Tian,W. W.,et al."The Kinematic Distances of SNR G16.7+0.1 and G15.9+0.2 by Analyzing H i Absorption Spectra".Publications of the Astronomical Society of the Pacific 131.1005(2019). |
入库方式： OAI收割
来源：国家天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。