http://arxiv.org/abs/1401.5600
[Abridged] We studied the size-surface brightness and the size-mass relations of a sample of 16 cluster elliptical galaxies morphologically selected in the cluster RDCS J0848+4453 at z=1.27. Our aim was to assess whether they have completed their mass growth at their redshift or significant mass and/or size growth can or must take place till z=0. As comparison samples of cluster ellipticals in the local universe we used the Coma Cluster sample of Jorgensen et al. and the WINGS survey sample. The comparison with the local Kormendy relation shows that the luminosity evolution due to the aging of the stellar content already assembled at z=1.27 brings them on the local relation. Moreover, they are on the size-mass relation of the local cluster ellipticals. These results imply that for a given mass the stellar mass at z~1.3 is distributed within these ellipticals according to the same stellar mass profile of local ellipticals. We find that a pure size evolution, even mild, is ruled out for our galaxies since it would bring them away from both the Kormendy and the size-mass relation. If an evolution of the effective radius takes place, this must be compensated by an increase of the luminosity and hence of the stellar mass of the galaxies to keep them on the local relations. We show that to remain on the Kormendy relation the stellar mass must increase as the effective radius. However, this mass growth is not sufficient to keep the galaxies on the size-mass relation for the same variation of effective radius. Thus, if we want to preserve the Kormendy relation we fail in satisfying the size-mass relation and vice versa. Hence, the combined analysis of the size-surface brightness relation with the size-mass relation leads to the result that these galaxies cannot growth further their stellar mass and/or change their structure.
Thu, 23 Jan 14
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