Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-06-20
Astronomy and Astrophysics
Astrophysics
6 pages, MNRAS main journal, accepted for publication
Scientific paper
10.1111/j.1365-2966.2007.12136.x
We derive deep luminosity functions (to $M_z=-15$) for galaxies in Abell 1835 ($z=0.25$) and AC 114 ($z=0.31$) and compare these with the local $z'$ luminosity function for 69 clusters. The data show that the faint-end upturn, the excess of galaxies above a single Schechter function at $M_z < -17$, does not exist in the higher redshift clusters. This suggests that the faint-end upturn galaxies have been created recently, by infall into clusters of star-forming field populations or via tidal disruption of brighter objects.^M
de Propris Roberto
Harsono Daniel
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