Early hierarchical formation of massive galaxies triggered by interactions

To address the problem concerning the early formation of stars in massive galaxies, we present the results of a semianalytic model of galaxy formation that includes a physical description of starbursts triggered by galaxy interactions. These originate from the destabilization of cold galactic gas that occurs in galaxy encounters, which in part feeds the accretion onto black holes that powers quasars and in part drives circumnuclear starbursts at redshifts z approximate to 2-4, preferentially in massive objects. This speeds up the formation of stars in massive galaxies at high redshifts without altering it in low-mass galactic halos. Thus, at intermediate z, approximate to1.5-2, we find that a considerable fraction of the stellar content of massive galaxies is already in place, at variance with the predictions of previous hierarchical models. The resulting high-z star formation rate and B-band luminosity functions and the luminosity and redshift distribution of galaxies in the K band at zless than or similar to2 are all in good agreement with the existing observations concerning the bright galaxy population.