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Expected Number Counts of Radio Galaxy Clusters
Wei Zhou
2002
Source PublicationChinese Journal of Astronomy and Astrophysics
ISSN1009-9271
Volume2Issue:2Pages:106
AbstractClusters of galaxies may contain radio sources if they still experience successive mergers at present. This has been confirmed by radio observations that about 30% of nearby clusters possess radio halos. We present a theoretical prediction of radio cluster counts using a semi-analytic approach which incorporates the empirical correlation between radio power and dynamical mass of clusters, and the cluster mass function described by the Press-Schechter formalism. The total population of radio clusters over the whole sky and their redshift distribution are given.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/53302
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wei Zhou. Expected Number Counts of Radio Galaxy Clusters[J]. Chinese Journal of Astronomy and Astrophysics,2002,2(2):106.
APA Wei Zhou.(2002).Expected Number Counts of Radio Galaxy Clusters.Chinese Journal of Astronomy and Astrophysics,2(2),106.
MLA Wei Zhou."Expected Number Counts of Radio Galaxy Clusters".Chinese Journal of Astronomy and Astrophysics 2.2(2002):106.
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