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Misgeld, Ingo (2011): Early-type stellar systems in nearby galaxy clusters: from dwarf galaxies to star clusters. Dissertation, LMU München: Fakultät für Physik

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Fig. 1.1. Luminosity functions of six different environments, i.e. the Virgo Cluster, the NGC 1407 Group,Trentham & Tullythe Coma I Group, the NGC 1023 Group, the Ursa Major Cluster and the Leo Group
Fig. 1.2. S´ersic surface brightness profiles (the total magnitude equals zero. The dotted line is offset by 0magnitude
Fig. 1.3. Left panel:(Las Campanas Observatory); insets: Hubble Space Telescope.UCDs and the nucleated dwarf galaxy from the left panel
Fig. 2.1. 45indicates the cluster core radius′×45′ (540×540 kpc at the cluster distance) image of the Hydra I cluster centred on NGC 3311,extracted from the Digital Sky Survey (DSS)
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Outline

The colour–magnitude relation of early-type galaxies Follow-up spectroscopy The Hydra I galaxy luminosity function Systematic radial velocity shifts Photometric and structural properties Kinematics Discussion and conclusions Fundamental scaling relations Galaxies as distance indicators The sizes of hot stellar systems

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