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  1. 1
    ... of the diffuse stellar populations in early-type galaxies if the number of clusters per unit stellar mass depends...
    Aportado por: SEDICI (UNLP)
    Articulo
  2. 2
    ... by assuming that the number of globular clusters per associated diffuse stellar mass t is a function of total...
    Aportado por: SEDICI (UNLP)
    Articulo
  3. 3
    ... and up to a limiting radius where the areal density of blue globular clusters falls to 30 per cent...
    Aportado por: SEDICI (UNLP)
    Articulo
  4. 4
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    ... candidate GCs. Our source list is greater than 90 per cent complete to a magnitude of i = 23.6, and has...
    Aportado por: SEDICI (UNLP)
    Articulo
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