Radio properties of the low surface brightness SNR G65.2+5.7
文献类型：期刊论文
| 作者 | Xiao, L.1; Reich, W.2; Fuerst, E.2; Han, J. L.1 |
| 刊名 | ASTRONOMY & ASTROPHYSICS
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| 出版日期 | 2009-09-01 |
| 卷号 | 503期号:3页码:827-836 |
| 关键词 | ISM: supernova remnants ISM: magnetic fields radio continuum: ISM radiation mechanisms: non-thermal |
| 英文摘要 | Context. SNR G65.2+5.7 is one of few supernova remnants (SNRs) that have been optically detected. It is exceptionally bright in X-rays and the optical [O III]-line. Its low surface brightness and large diameter ensure that radio observations of SNR G65.2+5.7 are technically difficult and thus have hardly been completed. Aims. Many physical properties of this SNR, such as spectrum and polarization, can only be investigated by radio observations. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000269727100018 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/8345]  |
| 专题 | 国家天文台_射电天文研究部 |
| 作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 2.Max Planck Inst Radioastron, D-53121 Bonn, Germany |
| 推荐引用方式 GB/T 7714 | Xiao, L.,Reich, W.,Fuerst, E.,et al. Radio properties of the low surface brightness SNR G65.2+5.7[J]. ASTRONOMY & ASTROPHYSICS,2009,503(3):827-836. |
| APA | Xiao, L.,Reich, W.,Fuerst, E.,&Han, J. L..(2009).Radio properties of the low surface brightness SNR G65.2+5.7.ASTRONOMY & ASTROPHYSICS,503(3),827-836. |
| MLA | Xiao, L.,et al."Radio properties of the low surface brightness SNR G65.2+5.7".ASTRONOMY & ASTROPHYSICS 503.3(2009):827-836. |
入库方式： OAI收割
来源：国家天文台
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