The evolution of the mass-size relation for early type galaxies from z~1 to the present: dependence on environment, mass-range and detailed morphology

Abstract

[abridged] We study the dependence of the galaxy size evolution on morphology, stellar mass and large scale environment for a sample of 298 group and 384 field quiescent early-type galaxies from the COSMOS survey, selected from z~1 to the present, and with masses $log(M/M_{\odot })>10.5$. The galaxy size growth depends on galaxy mass and early-type galaxy morphology, e.g., elliptical galaxies evolve differently than lenticular galaxies. At the low mass end -$10.5<Log(M/M_{\odot })<11$, ellipticals do not show strong size growth from $z\sim 1$ to the present (10% to 30% depending on the morphological classification). On the other end, massive ellipticals -log(M/M_\odot)>11.2$-approximatelydoubledtheirsize.Interestingly,lenticulargalaxiesdisplaydifferentbehavior:theyappearmorecompactonaverageandtheydoshowasizegrowthof\sim 60$log(M_h/M_\odot)<14$),i.e.,groupandfieldgalaxiesfollowthesametrends,whichisatvariancewithpredictionsfromcurrenthierarchicalmodelsthatshowacleardependenceofsizegrowthonhalomassformassiveellipticals-$log(M_*/M_\odot)>11.2$.

MNRAS in press, updated version after revision

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