Satellites of massive galaxies: the infalling pieces of the puzzle
Accretion of minor satellites has been postulated as the most likely mechanism to explain the significant size evolution of massive galaxies over cosmic time. A direct way of probing this scenario is to measure the frequency of satellites around massive galaxies at different redshifts. Here we present our study of satellites around massive galaxies
Mármol-Queraltó, E. et al.
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2013