The role of E+A and post-starburst galaxies - I. Models and model results
M. A. Falkenberg, R. Kotulla, U. Fritze

TL;DR
This paper models post-starburst galaxies to understand their role in galaxy evolution, revealing that spectral energy distribution comparisons are more effective than traditional criteria for identifying E+A galaxies.
Contribution
It introduces a new method for identifying post-starburst galaxies based on spectral energy distributions and explores the effects of metallicity and gas content on E+A galaxy prevalence.
Findings
Traditional E+A criteria exclude many post-starburst galaxies
Higher E+A galaxy numbers in the early universe are due to metallicity and gas content, not just starbursts
Normal galaxies can exhibit Hdelta-strong phases early in their evolution
Abstract
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 late- to 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…
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