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The galaxy formation model
On the impact of empirical and theoretical star formation laws on galaxy formation
Cosmic evolution of the atomic and molecular gas content of galaxies and scaling relations
Predictions for the CO emission of galaxies from a coupled simulation of galaxy formation and photon dominated regions
A dynamical model of supernova feedback: gas outflows from the interstellar medium
Conclusions
Non-exponential star formation laws and their application to a numerical model
The CO line and IR luminosity
Radial profiles of the stellar and dark matter components
The recycle fraction and yield of different stellar populations.

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