The role of E+A and post-starburst galaxies I. Models and model results

Different compositions of galaxy types in the field in comparison to galaxy clusters as described by the morphology-density relation in the local universe is interpreted as a result of transformation processes from lateto early-type galaxies. This interpretation is supported by the Butcher-Oemler effect. We investigate E+A galaxies as an intermediate state between late-type galaxies in low density environments and early-type galaxies in high density environment to constrain the possible transformation processes. For this purpose we model a grid of post-starburst galaxies by inducing a burst and/ or a halting of star formation on the normal evolution of spiral galaxies with our galaxy evolution code GALEV. From our models we find that the common E+A criteria exclude a significant number of post-starburst galaxies and propose that comparing their spectral energy distributions leads to a more sufficient method to investigate post-starbust galaxies. We predict that a higher number of E+A galaxies in the early universe can not be ascribed solely to a higher number of starburst, but is a result of a lower metallicity and a higher burst strength due to more gas content of the galaxies in the early universe. We find that even galaxies with a normal evolution without a starburst have a Hδ-strong phase at early galaxy ages.