Radio spectral properties and the magnetic field of the SNR S147
文献类型:期刊论文
作者 | Xiao, L.1; Fuerst, E.2; Reich, W.2; Han, J. L.1 |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2008-05-01 |
卷号 | 482期号:3页码:783-792 |
关键词 | ISM : supernova remnants radio continuum : ISM techniques : polarimetric |
英文摘要 | Context. S147 is a large faint shell-type supernova remnant ( SNR) known for its remarkable spectral break at cm-wavelength, which is an important physical property to characterize SNR evolution. However, the spectral break is based on radio observations with limited precision. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000255268000012 |
源URL | [http://ir.bao.ac.cn/handle/114a11/7457] ![]() |
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.,Fuerst, E.,Reich, W.,et al. Radio spectral properties and the magnetic field of the SNR S147[J]. ASTRONOMY & ASTROPHYSICS,2008,482(3):783-792. |
APA | Xiao, L.,Fuerst, E.,Reich, W.,&Han, J. L..(2008).Radio spectral properties and the magnetic field of the SNR S147.ASTRONOMY & ASTROPHYSICS,482(3),783-792. |
MLA | Xiao, L.,et al."Radio spectral properties and the magnetic field of the SNR S147".ASTRONOMY & ASTROPHYSICS 482.3(2008):783-792. |
入库方式: OAI收割
来源:国家天文台
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