Virial scaling of massive dark matter halos: Why clusters prefer a high normalization cosmology

Astrophysical Journal

Volumn 672, Issue 1, 2008, Pages 122-137

  Evrard, A E ^a,b   Bialek, J ^a   Busha, M ^a   White, M ^b   Habib, S ^c   Heitmann, K ^c   Warren, M ^c   Rasia, E ^a,d,e,f   Tormen, G ^e   Moscardini, L ^d,g   Power, C ^h   Jenkins, A R ⁱ   Gao, L ⁱ   Frenk, C S ⁱ   Springel, V ^j   White, S D M ^j   Diemand, J ^f,k  

^a UNIVERSITY OF MICHIGAN   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c LOS ALAMOS NATIONAL LABORATORY   (United States)

^d UNIVERSITY OF BOLOGNA   (Italy)

^e UNIVERSITY OF PADOVA   (Italy)

^f Chandra ^*

^g INFN SEZIONE DI BOLOGNA   (Italy)

^h SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

ⁱ DURHAM UNIVERSITY   (United Kingdom)

^j MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^k University of California at Santa Cruz   (United States)

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Author keywords

Cosmology: miscellaneous; Cosmology: theory; Dark matter; Galaxies: clusters: general; Gravitation; Intergalactic medium

Indexed keywords

EID: 40249092899     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/521616     Document Type: Article

References (117)