Why does the clustering of haloes depend on their formation history?

Monthly Notices of the Royal Astronomical Society

Volumn 377, Issue 1, 2007, Pages 234-244

  Sandvik, H B ^a   Moller O ^a   Lee, J ^b   White, S D M ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b Seoul National University   (South Korea)

Author keywords

Cosmology: theory; Galaxies: clusters: general; Galaxies: haloes; Large scale structure of Universe; Methods: statistical

Indexed keywords

GALAXIES;

CLUSTERINGS; COSMOLOGY: THEORY; EXCURSION SET; GALAXIES: CLUSTERS: GENERAL; GALAXY:HALO; INITIAL DENSITY; LARGE SCALE STRUCTURE OF UNIVERSE; LOW-MASS; METHODS:STATISTICAL; N-BODY SIMULATION;

MONTE CARLO METHODS;

EID: 34247874605     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11595.x     Document Type: Article

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