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Galaxy groups in the 2dF Galaxy Redshift Survey : the number density of groups

Author
EKE, V. R1 ; BAUGH, Carlton M1 ; COLE, Shaun1 ; FRENK, Carlos S1 ; NAVARRO, Julio F2
[1] Department of Physics, University of Durham, South Road, Durham DH1 3LE, United Kingdom
[2] Department of Physics and Astronomy, University of Victoria, Victoria, BC, V8P 5C2, Canada
Source

Monthly Notices of the Royal Astronomical Society. 2006, Vol 370, Num 3, pp 1147-1158, 12 p ; ref : 68 ref

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Blackwell Science, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
galaxies: clusters: general galaxies: haloes large-scale structure of Universe
Keyword (fr)
Abondance Amas galaxies Catalogue astronomique Correction Déplacement vers le rouge Fluctuation densité Fonction masse Galaxies Groupe galaxies Luminosité Modèle Percolation Rapport masse luminosité Relation Tully Fisher Simulation numérique Sphère Structure grande échelle Système n corps Théorie linéaire Vitesse rotation Halo galaxies
Keyword (en)
Abundance Galaxy clusters Astronomical catalogues Corrections Red shift Density fluctuation Mass function Galaxies Galaxy groups Luminosity Models Percolation Mass to light ratio Tully Fisher relation Digital simulation Spheres Large-scale structure N body system Linear theory Rotation speed Galaxy halo
Keyword (es)
Fluctuación densidad Función masa Modelo Relación masa luminosidad Relación Tully Fisher Sistema n cuerpos Teoría lineal Velocidad rotación Halo galaxia
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
17982601

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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