Impact of baryon physics on dark matter structures: A detailed simulation study of halo density profiles

Monthly Notices of the Royal Astronomical Society

Volumn 405, Issue 4, 2010, Pages 2161-2178

  Duffy, Alan R ^a,b,c   Schaye, Joop ^b   Kay, Scott T ^a   Vecchia, Claudio Dalla ^b,d   Battye, Richard A ^a   Booth, C M ^b  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

^b LEIDEN UNIVERSITY   (Netherlands)

^c UNIVERSITY OF WESTERN AUSTRALIA   (Australia)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Dark matter; Galaxies: haloes; Galaxies: structure; Gravitation; Hydrodynamics; Methods: numerical

Indexed keywords

GALAXIES; HADRONS; ISOTHERMS; NUMERICAL METHODS; STARS;

ACTIVE GALACTIC NUCLEI; BACK REACTION; DARK MATTER; DARK MATTER HALOS; DENSITY PROFILE; GALAXIES:STRUCTURE; GALAXY:HALO; METHOD: NUMERICAL; SIMULATION STUDIES; SYSTEMATIC UNCERTAINTIES;

GRAVITATION;

EID: 77955038943     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16613.x     Document Type: Article

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