
In this thesis, radial colour and line strength gradients are investigated, and corresponding stellar population gradients are modelled. Together with the gradients, the morphology of the galaxies in optical and near-infrared colours is analyzed. When investigated in detail, every elliptical galaxy has its own special morphology, but nevertheless the class of ellipticals has a large number of properties in common. We will list here the most important conclusions of this work ... .... Zie: Summary
Elliptische sterrenstelsels, Structuur, Proefschriften (vorm)
Elliptische sterrenstelsels, Structuur, Proefschriften (vorm)
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