Properties of galaxy groups in the Sloan Digital Sky Survey - I. The dependence of colour, star formation and morphology on halo mass
- Author
- WEINMANN, Simone M1 2 ; VAN DEN BOSCH, Frank C1 3 ; XIAOHU YANG4 ; MO, H. J4
[1] Department of Physics, Swiss Federal Institute of Technology, ETH Honggerberg, 8093 Zurich, Switzerland
[2] Institute for Theoretical Physics, University of Zurich, 8057 Zurich, Switzerland
[3] Max-Planck-Institute for Astronomy, Konigstuhl 17, 69117 Heidelberg, Germany
[4] Department ofAstronomy, University of Massachussets, 710 North Pleasant Street, Amherst, MA 01003-9305, United States - Source
Monthly Notices of the Royal Astronomical Society. 2006, Vol 366, Num 1, pp 2-28, 27 p ; ref : 1 p.1/4
- 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: evolution galaxies: general galaxies: haloes galaxies: statistics methods: statistical
- Keyword (fr)
- Amas galaxies Catalogue astronomique Corrélation Couleur Estimateur Etude ciel Formation galaxies Formation stellaire Galaxies compagnons Galaxies premier type Galaxies type avancé Groupe galaxies Luminosité Morphologie Méthode statistique Taux formation Evolution galaxies Halo galaxies
- Keyword (en)
- Galaxy clusters Astronomical catalogues Correlations Color Estimator Sky surveys Galaxy formation Star formation Satellite galaxies Early type galaxies Late type galaxies Galaxy groups Luminosity Morphology Statistical method Formation rate Galaxy evolution Galaxy halo
- Keyword (es)
- Estimador Galaxias satélite Galaxias primer tipo Galaxias tipo avanzado Método estadístico Grado formación Evolución galaxias Halo galaxia
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17575461
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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DOI
10.1111/j.1365-2966.2005.09865.x 
https://dx.doi.org/10.1111/j.1365-2966.2005.09865.x
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