On the Size and Comoving Mass Density Evolution of Early-Type Galaxies

Details On the Size and Comoving Mass Density Evolution of Early-Type Galaxies On the Size and Comoving Mass Density Evolution of Early-Type Galaxies

2009-03-27

arxiv.org/abs/0903.4857v3

Astrophys.J.698:1232-1243,2009

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

Accepted for publication in ApJ (13 pages, 5 figures), small changes to match journal version

Scientific paper

10.1088/0004-637X/698/2/1232

We present a simple, empirically motivated model that simultaneously predicts the evolution of the mean size and the comoving mass density of massive early-type galaxies from z=2 to the present. First we demonstrate that some size evolution of the population can be expected simply due to the continuous emergence of early-type galaxies. SDSS data reveal that in the present-day universe more compact early-type galaxies with a given dynamical mass have older stellar populations. In contrast, at a given stellar velocity dispersion, SDSS data show that there is no relation between size and age, which implies that the velocity dispersion can be used to estimate the epoch at which galaxies stopped forming stars, turning into early-type galaxies. Applying such a 'formation' criterion to a large sample of nearby early-type galaxies, we predict the redshift evolution in the size distribution and the comoving mass density. The resulting evolution in the mean size is roughly half of the observed evolution. Then we include a prescription for the merger histories of galaxies between the 'formation' redshift and the present, based on cosmological simulations of the assembly of dark matter halos. Such mergers after the transformation into an early-type galaxy are presumably dissipationless ('dry'), where the increase in size is expected to be approximately proportional to the increase in mass. This model successfully reproduces the observed evolution since z~2 in the mean size and in the comoving mass density of massive early-type galaxies. We conclude that the recently measured, substantial size evolution of early-type galaxies can be explained by the combined effect of the continuous emergence of galaxies as early types and their subsequent growth through dry merging.

Affiliated with

Also associated with

No associations

Rating

On the Size and Comoving Mass Density Evolution of Early-Type Galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with On the Size and Comoving Mass Density Evolution of Early-Type Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Size and Comoving Mass Density Evolution of Early-Type Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-21865