Non-spherical similarity solutions for dark halo formation

Monthly Notices of the Royal Astronomical Society

Volumn 414, Issue 4, 2011, Pages 3044-3051

  Vogelsberger, Mark ^a   Mohayaee, Roya ^b   White, Simon D M ^c  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b CNRS   (France)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Dark matter

Indexed keywords

GALAXIES; PHASE SPACE METHODS;

DARK MATTER; HALO FORMATION; INITIAL CONDITIONS; NON-SPHERICAL; POWER-LAW; SELF-SIMILAR; SIMILARITY INDICES; SIMILARITY SOLUTION; THREE DIMENSIONAL SIMULATIONS; VELOCITY ANISOTROPY;

ANISOTROPY;

EID: 79959853685     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18605.x     Document Type: Article

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