The HI absorption distance of HESS J1943+213 favours its extragalactic nature
文献类型：期刊论文
| 作者 | Leahy, D. A.1; Tian, W. W.2 |
| 刊名 | ASTRONOMY & ASTROPHYSICS
 |
| 出版日期 | 2012-03-01 |
| 卷号 | 539 |
| 关键词 | methods: data analysis ISM: supernova remnants cosmic rays |
| 英文摘要 | Context. The H.E.S.S. Collaboration dicovered a new TeV point-like source HESS J1943+213 in the Galactic plane and suggested three possible low-energy-band counterparts: a gamma-ray binary, a pulsar wind nebula ()PWN), or a BL Lacertae object. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000303262000135 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6238]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | 1.Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada 2.CAS, Natl Astron Observ, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Leahy, D. A.,Tian, W. W.. The HI absorption distance of HESS J1943+213 favours its extragalactic nature[J]. ASTRONOMY & ASTROPHYSICS,2012,539. |
| APA | Leahy, D. A.,&Tian, W. W..(2012).The HI absorption distance of HESS J1943+213 favours its extragalactic nature.ASTRONOMY & ASTROPHYSICS,539. |
| MLA | Leahy, D. A.,et al."The HI absorption distance of HESS J1943+213 favours its extragalactic nature".ASTRONOMY & ASTROPHYSICS 539(2012). |
入库方式： OAI收割
来源：国家天文台
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