A Simple Model for the Size Evolution of Elliptical Galaxies

We use semianalytical modeling of galaxy formation to predict the redshift-size evolution of elliptical galaxies. Using a simple model in which relative sizes of elliptical galaxies of a given mass correlate with the fraction of stars formed in a starburst during a major merger event, we are able to reproduce the observed redshift-size evolution. The size evolution is a result of the amount of cold gas available during the major merger. Mergers at high redshifts are gas-rich and produce ellipticals with smaller sizes. In particular, we find a power-law relation between the sizes at different redshifts, with the power-law index giving a measure of the relative amount of dissipation during the mergers that lead to the formation of an elliptical. The size evolution is found to be stronger for more massive galaxies as they involve more gas at high redshifts when they form, compared to less massive ellipticals. Local ellipticals more massive than 5 x 10 super(11) M sub( )will be approximately 4 times larger than their counterparts at z = 2. Our results indicate that the scatter in the size of similar massive present-day elliptical galaxies is a result of their formation epoch, with smaller ellipticals being formed earlier.