Evidence of turbulence-like universality in the formation of galaxy-sized dark matter haloes

Astronomy and Astrophysics

Volumn 487, Issue 2, 2008, Pages 445-451

  Caretta, C A ^a,b   Rosa, R R ^b   De Campos Velho, H F ^b   Ramos, F M ^b   Makler, M ^c  

^a UNIVERSITY OF GUANAJUATO   (Mexico)

^b INSTITUTO NACIONAL DE PESQUISAS ESPACIAIS   (Brazil)

^c CENTRO BRASILEIRO DE PESQUISAS FÍSICAS   (Brazil)

Author keywords

Galaxies: evolution; Galaxies: structure; Gravitation; Methods: N body simulations; Methods: statistical; Turbulence

Indexed keywords

CHLORINE COMPOUNDS; CLUSTER ANALYSIS; FLOW OF SOLIDS; GRAVITATION; POWER SPECTRUM; SPECTRUM ANALYSIS; TURBULENCE;

BOUNDEDNESS; CLUSTERS OF GALAXIES; DARK MATTER; EN ERGY SPECTRUM; GALAXIES: EVOLUTION; GALAXIES: STRUCTURE; GRAVITATIONAL CLUSTERING; GRAVITATIONAL POTENTIAL ENERGY; KOLMOGOROV; METHODS: N-BODY SIMULATIONS; METHODS: STATISTICAL; PHYSICAL PROCESSES; POWER LAWS; RED SHIFTING; SIMULATION DATA; TURBULENT PROCESSES;

GALAXIES;

EID: 48849086009     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079105     Document Type: Article

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