中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Polarization observations of SNR G156.2+5.7 at lambda 6 cm

文献类型:期刊论文

作者Xu, J. W.; Han, J. L.; Sun, X. H.; Reich, W.; Xiao, L.; Reich, P.; Wielebinski, R.
刊名ASTRONOMY & ASTROPHYSICS
出版日期2007-08-01
卷号470期号:3页码:969-975
关键词ISM : supernova remnants radio continuum : ISM polarization ISM : magnetic fields
英文摘要Context. G156.2+5.7 is a large supernova remnant (SNR) first discovered in the ROSAT X-ray survey due to its exceptional high X-ray brightness. Subsequently detailed X-ray, optical and Ha studies of this SNR were made, but radio observations are rare because of its low surface brightness and large size.
收录类别SCI
语种英语
WOS记录号WOS:000248190700016
源URL[http://ir.bao.ac.cn/handle/114a11/7300]  
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
Xu, J. W.,Han, J. L.,Sun, X. H.,et al. Polarization observations of SNR G156.2+5.7 at lambda 6 cm[J]. ASTRONOMY & ASTROPHYSICS,2007,470(3):969-975.
APA Xu, J. W..,Han, J. L..,Sun, X. H..,Reich, W..,Xiao, L..,...&Wielebinski, R..(2007).Polarization observations of SNR G156.2+5.7 at lambda 6 cm.ASTRONOMY & ASTROPHYSICS,470(3),969-975.
MLA Xu, J. W.,et al."Polarization observations of SNR G156.2+5.7 at lambda 6 cm".ASTRONOMY & ASTROPHYSICS 470.3(2007):969-975.

入库方式: OAI收割

来源:国家天文台

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