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    • We present the distribution of virial masses for nearby galaxy clusters, as obtained from a data set of 75 clusters, each having at least 20 galaxy members with measured redshifts within 1.5/h Mpc. After having accounted for problems of incompleteness of the data set, we fitted a power law to the cluster mass distribution.


    Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11368/1695150

    Titolo: The Mass Function of Nearby Galaxy Clusters
    Autori: 
    GIRARDI, MARISA
    MARDIROSSIAN, FABIO
    MEZZETTI, MARINO
    mostra contributor esterni 
    Data di pubblicazione: 1993
    Rivista: 
    THE ASTROPHYSICAL JOURNAL  
    Abstract: We present the distribution of virial masses for nearby galaxy clusters, as obtained from a data set of 75 clusters, each having at least 20 galaxy members with measured redshifts within 1.5/h Mpc. After having accounted for problems of incompleteness of the data set, we fitted a power law to the cluster mass distribution.
    Handle: http://hdl.handle.net/11368/1695150
    Digital Object Identifier (DOI): 10.1086/186900
    URL: http://adsabs.harvard.edu/abs/1993ApJ...411L..13B
    Appare nelle tipologie:1.1 Articolo in Rivista

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