Non-Gaussian cosmic microwave background temperature fluctuations from peculiar velocities of clusters

Monthly Notices of the Royal Astronomical Society

Volumn 328, Issue 2, 2001, Pages 669-677

  Yoshida, Naoki ^a,c   Sheth, Ravi K ^b   Diaferio, Antonaldo ^d  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b NASA FERMILAB ASTROPHYSICS CENTER   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d NONE

Author keywords

Cosmic microwave background; Galaxies: Clusters: General; Gravitation; Large scale structure of Universe; Methods: N body simulations

Indexed keywords

DISPERSIONS; GALAXIES; GAUSSIAN DISTRIBUTION; GAUSSIAN NOISE (ELECTRONIC); GRAVITATION; KINEMATICS; TEMPERATURE DISTRIBUTION;

COSMIC MICROWAVES BACKGROUND; GALAXIES: CLUSTERS: GENERAL; HALO MASS; LARGE SCALE STRUCTURE OF UNIVERSE; METHODS:N-BODY SIMULATIONS; NON-GAUSSIAN; OPTICAL DEPTH; PEAK HEIGHT; SUNYAEV-ZELDOVICH EFFECTS; TEMPERATURE FLUCTUATION;

COSMOLOGY;

EID: 0011063333     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04899.x     Document Type: Article

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