Titlebook: Astrophysics; An Introduction to T Karl-Heinz Spatschek Textbook 20241st edition The Editor(s) (if applicable) and The Author(s), under exc

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Galaxies (Milky Way) and then turn to the classification of the abundance of galaxies [3, 36]. Subsequently, we summarize evidence for the existence of Dark Matter and introduce the important new field of numerical modeling using .CDM models. This ultimately leads to the question of the embedding of galaxie

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Homogeneous Cosmologysical” form, in which the cosmos is assumed to be completely homogeneous and isotropic. The Robertson-Walker metric is used in this case. Inhomogeneous cosmology takes into account density and temperature fluctuations. We begin with homogeneous cosmology.

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