The relation between halo shape, velocity dispersion and formation time

Monthly Notices of the Royal Astronomical Society

Volumn 407, Issue 1, 2010, Pages 581-589

  Ragone Figueroa, C ^a,b   Plionis, M ^c,d   Merchan M ^a,b   Gottlober S ^e   Yepes, G ^f  

^a Instituto de Astronomia Teorica y Experimental   (Argentina)

^b Facultad de Ciencias Naturales e Instituto M Lillo   (Argentina)

^c NATIONAL OBSERVATORY OF ATHENS   (Greece)

^d INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^e ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^f UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

Author keywords

Dark matter; Galaxies: clusters: general; Galaxies: haloes; Methods: numerical

Indexed keywords

DISPERSIONS; DYNAMICS; NUMERICAL METHODS; VELOCITY;

DARK MATTER; DYNAMIC CORRELATION; FORMATION TIME; GALAXIES: CLUSTERS: GENERAL; GALAXY:HALO; METHOD: NUMERICAL; SHAPE DYNAMICS; SLOAN DIGITAL SKY SURVEY; SURVEY DATA; VELOCITY DISPERSION;

GALAXIES;

EID: 77956403181     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16935.x     Document Type: Article

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