Properties of galaxy haloes in clusters and voids

Monthly Notices of the Royal Astronomical Society

Volumn 332, Issue 1, 2002, Pages 7-20

  Antonuccio Delogu, V ^a,f   Becciani, U ^a   Van Kampen, E ^b   Pagliaro, A ^c   Romeo, A B ^d   Colafrancesco, S ^g   Germana A ^a   Gambera, M ^e  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b UNIVERSITY OF EDINBURGH   (United Kingdom)

^c SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^d CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^e Liceo Science Statale E Majorana   (Italy)

^f THEORETICAL ASTROPHYSICS CENTER   (Denmark)

^g NONE

Author keywords

Galaxies: formation; Galaxies: haloes; Largescale structure of Universe; Methods: N body simulations

Indexed keywords

GRAVITATION; PROBABILITY DISTRIBUTIONS;

FORMATION AND EVOLUTIONS; GALAXY FORMATIONS; GALAXY:HALO; HIGH RESOLUTION; ISOTHERMAL SPHERES; LARGE SCALE STRUCTURE OF UNIVERSE; METHODS:N-BODY SIMULATIONS; N-BODY SIMULATION; PROPERTY; SPHERE MODEL;

GALAXIES;

EID: 0041847224     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05258.x     Document Type: Article

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