The supercluster-void network - III. The correlation function as a geometrical statistic

Monthly Notices of the Royal Astronomical Society

Volumn 289, Issue 4, 1997, Pages 813-823

  Einasto, J ^a   Einasto, M ^a   Frisch, P ^b   Gottlober S ^c   Muller V ^c   Saar, V ^a   Starobinsky, A A ^d   Tucker, D ^c,e  

^a TARTU OBSERVATORY   (Estonia)

^b UNIVERSITY OF GÖTTINGEN   (Germany)

^c ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^d LANDAU INSTITUTE FOR THEORETICAL PHYSICS   (Russian Federation)

^e FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

Author keywords

Cosmology: Theory; Galaxies: Clusters: General; Large scale structure of Universe; Methods: Numerical

Indexed keywords

GALAXIES; GEOMETRY; NUMERICAL METHODS; RANDOM ERRORS;

CORRELATION FUNCTION; COSMOLOGY: THEORY; DISTRIBUTION OF CLUSTER; GALAXIES: CLUSTERS: GENERAL; LARGE SCALE STRUCTURE OF UNIVERSE; LARGE-SCALES; METHOD: NUMERICAL; POWER-SPECTRA; SUPERCLUSTERS; VOID NETWORKS;

POWER SPECTRUM;

EID: 0010656355     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/289.4.813     Document Type: Article

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