The halo density profiles with non-standard N-body simulations

Monthly Notices of the Royal Astronomical Society

Volumn 338, Issue 1, 2003, Pages 156-164

  D'Onghia, E ^a,b   Firmani, C ^c,d   Chincarini, G ^c,e  

^a UNIVERSITY OF MILAN   (Italy)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c INAF OSSERVATORIO ASTRONOMICO DI BRERA   (Italy)

^d UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^e UNIVERSITY OF MILANO BICOCCA   (Italy)

Author keywords

Cosmology: Miscellaneous; Dark matter; Galaxies: Haloes

Indexed keywords

CLUSTER COMPUTING; CODES (SYMBOLS); GALAXIES;

COLLISIONLESS; COSMOLOGY: MISCELLANEOUS; DARK MATTER; DENSITY PROFILE; GALAXIES CLUSTERS; GALAXY:HALO; INITIAL CONDITIONS; N-BODY SIMULATION; NUMERICAL PROCEDURES; SINGLE HALO;

COSMOLOGY;

EID: 0043195609     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06029.x     Document Type: Article

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