Comparisons between isothermal and nfw mass profiles for strong-lensing galaxy clusters

Astrophysical Journal

Volumn 685, Issue 1, 2008, Pages 70-82

  Shu, Chenggang ^a,b,c   Zhou, Binglu ^a,b   Bartelmann, Matthias ^b   Comerford, Julia M ^d   Huang, J S ^e   Mellier, Yannick ^f  

^a SHANGHAI NORMAL UNIVERSITY   (China)

^b UNIVERSITY OF HEIDELBERG   (Germany)

^c CHINESE ACADEMY OF SCIENCES   (China)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

Author keywords

Dark matter; Galaxies: clusters: individual (MS 2137, A370); Gravitational lensing

Indexed keywords

EID: 53549126610     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/590049     Document Type: Article

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