The cluster distribution as a test of dark matter models - III. the cluster velocity field

Monthly Notices of the Royal Astronomical Society

Volumn 282, Issue 2, 1996, Pages 384-400

  Moscardini, L ^a   Branchini, E ^b,c   Tini Brunozzi, P ^d,e   Borgani, S ^b,e   Plionis, M ^b,f   Coles, P ^g  

^a UNIVERSITY OF PADOVA   (Italy)

^b SISSA   (Italy)

^c DURHAM UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF PERUGIA   (Italy)

^e INFN SEZIONE DI PERUGIA   (Italy)

^f NATIONAL OBSERVATORY OF ATHENS   (Greece)

^g QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

Author keywords

Cosmology: theory; Dark matter; Galaxies: clusters: general; Galaxies: formation; Large scale structure of universe

Indexed keywords

COSMOLOGY; GALAXIES;

BULK FLOW; CLUSTER DISTRIBUTIONS; COSMOLOGY: THEORY; DARK MATTER; FREQUENCY DISTRIBUTIONS; GALAXIES: CLUSTERS: GENERAL; GALAXY FORMATIONS; LARGE SCALE STRUCTURE OF UNIVERSE; VELOCITIES DATA; VELOCITY FIELD;

VELOCITY;

EID: 0002317685     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/282.2.384     Document Type: Article

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