Early type galaxies in the hierarchical universe

Any realistic theory of galaxy formation must be set in the context of a model for the formation of structure in the universe. We describe a powerful approach -- semi-analytic modelling -- that combines a set of simple rules describing the gas processes involved in galaxy formation with a scheme to follow the hierarchical growth of dark matter haloes. Surprisingly few free parameters are required to specify the model, and these are fixed with reference to a subset of local observational data. The model produces the full star formation history of a galaxy, allowing a wide range of predictions to be made. We review some of the successes of the models, namely the star formation history of the universe and the evolution of galaxy clustering, before focusing our attention on early-type galaxies. We discuss the observational evidence against the classical picture in which early-type galaxies form at some arbitrarily high redshift in a single monolithic collapse and burst of star formation. The alternative scenario in which spheroidal systems are formed by the merger of disk galaxies is outlined. We review some of the predictions of this model, namely the colour-magnitude relation, the faint counts and the evolution of cluster membership