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The Interplay between ISM, Star Formation and Galaxy Evolution
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Journal Article
The Interplay between ISM, Star Formation and Galaxy Evolution
2004
Overview
Issue Title: From Observations to Self-Consistent Modelling of the ISM in Galaxies I present a model for the formation and evolution of a massive disk galaxy, within a growing dark halo whose mass evolves according to cosmological simulations of structure formation. The galactic evolution is simulated with a new 3D chemo-dynamical code, including dark matter, stars and a multi-phase ISM. We follow the evolution from redshift z = 4.85 until the present epoch. The energy release by massive stars and supernovae prevents a rapid collapse of the baryonic matter and delays the maximum star formation until redshift z [asymptotically =] 1. The galaxy forms radially from inside-out and vertically from top-to-bottom. The feedback of stars leads to turbulent motions and large-scale flows in the ISM. As one result the galactic disk is significantly enriched by chemical elements synthesized in bulge stars.[PUBLICATION ABSTRACT]
Publisher
Springer Nature B.V
Subject
