• Aiuto
  • Sfoglia

    • 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 interni: GIRARDI, MARISA
    MARDIROSSIAN, FABIO
    MEZZETTI, MARINO
    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

    File in questo prodotto:
    Non ci sono file associati a questo prodotto.
    • Citazioni
    • ND
    • ND
    • ND

    I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
     
     
     
    ©2014 University of Trieste dove siamo Privacy
    Piazzale Europa,1 34127 Trieste, Italia - Tel. +39 040.558.7111 - P.IVA 00211830328 - C.F. 80013890324 - P.E.C.: ateneo@pec.units.it
     Copyright © 2017