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Gobat, Raphael (2009): Evolution of early-type galaxies in field and cluster environments at z~1. Dissertation, LMU München: Fakultät für Physik

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Figure 1.1: Hubble “tuning-fork” sequence showing, from left to right, elliptical galaxies(E), S0 galaxies and spiral galaxies, both normal (S) and barred (SB)
Figure 1.2: (U − V ) − MV color-magnitude relation of galaxies in the Coma cluster. El-liptical galaxies are shown in red, S0 galaxies in green and late-type galaxies in blue
Figure 1.3: Projections of the fundamental plane: the relation between the radius and meansurface brightness (top left), the Faber-Jackson ([1976]) relation between luminosity andvelocity dispersion (top right), the relation between mean surface brightness
Figure 1.4: Monolithic model of galaxy formation (left), where galaxies form in isolationand their evolution is dependent mostly on initial conditions, and the hierarchical model(right), where galaxies form and evolve through successive mergers of smaller
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