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- W3099110966 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 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 Hdelta-strong phase at early galaxy ages." @default.
- W3099110966 created "2020-11-23" @default.
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- W3099110966 date "2009-08-21" @default.
- W3099110966 modified "2023-09-25" @default.
- W3099110966 title "The role of E+A and post-starburst galaxies - I. Models and model results" @default.
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- W3099110966 doi "https://doi.org/10.1111/j.1365-2966.2009.14416.x" @default.
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