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Radio properties of the low surface brightness SNR G65.2+5.7
Xiao, L.1; Reich, W.2; Fuerst, E.2; Han, J. L.1
2009-09-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume503Issue:3Pages:827-836
AbstractContext. 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.
KeywordIsm: Supernova Remnants Ism: Magnetic Fields Radio Continuum: Ism Radiation Mechanisms: Non-thermal
DOI10.1051/0004-6361/200911706
Indexed BySCI
Language英语
WOS IDWOS:000269727100018
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8345
Collection射电天文研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Max Planck Inst Radioastron, D-53121 Bonn, Germany
Recommended Citation
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.
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