Thermal and non-thermal emission in the Cygnus X region

	Thermal and non-thermal emission in the Cygnus X region
	Xu, W. F.1,2; Gao, X. Y.2; Han, J. L.2; Liu, F. S.1
刊名	ASTRONOMY & ASTROPHYSICS
	2013-11-01
卷号	559
关键词	radio continuum: ISM ISM: supernova remnants HII regions
英文摘要	Context. Radio continuum observations detect non-thermal synchrotron and thermal bremsstrahlung radiation. Separation of the two different emission components is crucial for studying the properties of the Galactic interstellar medium. The Cygnus X region is one of the most complex areas in the radio sky, which contains a number of massive stars and HII regions on the diffuse thermal and non-thermal background. More supernova remnants (SNRs) are expected to be discovered.
收录类别	SCI
语种	英语
WOS记录号	WOS:000327847200081
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/5938]
专题	国家天文台_射电天文研究部
作者单位	1.Shenyang Normal Univ, Coll Phys Sci & Technol, Shenyang 110034, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式 GB/T 7714	Xu, W. F.,Gao, X. Y.,Han, J. L.,et al. Thermal and non-thermal emission in the Cygnus X region[J]. ASTRONOMY & ASTROPHYSICS,2013,559.
APA	Xu, W. F.,Gao, X. Y.,Han, J. L.,&Liu, F. S..(2013).Thermal and non-thermal emission in the Cygnus X region.ASTRONOMY & ASTROPHYSICS,559.
MLA	Xu, W. F.,et al."Thermal and non-thermal emission in the Cygnus X region".ASTRONOMY & ASTROPHYSICS 559(2013).