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Guo, Qi (2009): Galaxy Formation and Evolution in a LCDM Universe. Dissertation, LMU München: Fakultät für Physik

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Figure

Figure 1.2: Substructures in a cluster (Springel et al. 2005).
Figure 2.1:The specific rate of formation of galaxies through major mergers as aformed through a major merger if its two largest progenitors in the preceding MillenniumRun output differ by less than a factor of 3 in stellar mass
Figure 2.2:The relation between the stellar mass of galaxies and their specific for-mation rate through major mergers
Figure 2.3:Dimensionless mean growth rates for galaxies as a function of redshiftfor the 7 different stellar mass bins of Fig
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