Titlebook: Dark Matter in Astro- and Particle Physics; Proceedings of the I H. V. Klapdor-Kleingrothaus,R. D. Viollier Conference proceedings 2002 Spr

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Aufgaben aus der Theoretischen Physikosmic structures. Extra-heating from Supernovae following star formation in the galaxies which built up the groups/clusters can account for the observations in a . dominated or in a critical Universe, while they fail to provide the observed X-ray properties of galaxy groups in open Universes or in models with a high fraction of hot dark matter ..

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Dark Matter and Baryons in Groups and Clusters of Galaxiesosmic structures. Extra-heating from Supernovae following star formation in the galaxies which built up the groups/clusters can account for the observations in a . dominated or in a critical Universe, while they fail to provide the observed X-ray properties of galaxy groups in open Universes or in models with a high fraction of hot dark matter ..

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held in Cape Town, South Africa, in the period 4-9 February 2002. This majestic natural area was the site of the first conference of this series (hosted since 1996 in Heidelberg) to be held outside of Germany. Dark Matter has become one of the most exciting and central fields of as- trophysics, par

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Aufgaben aus der Theoretischen Physikve output of those objects, and in some cases, for formation and acceleration of powerful relativistic jets. This paper outlines our current understanding of the structure of AGN, and summarizes the observational evidence for black holes in those objects.

Canyon

Aufgaben aus der Theoretischen Physiked microlensing events may make up around 20% of the dark matter in the Milky Way, or may indicate an otherwise undetected component of the Large Magellanic Cloud. Several new pieces of work lend support to both possibilities, leaving the answer uncertain.

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Aufgaben aus der Technischen Mechaniksults on the power spectrum and two-point correlation correlation function from the 2dF and REFLEX surveys, highlighting the advantage of X-ray clusters in the comparison to cosmological models, given their easy-to-understand mass selection function. I also mention recent measurements of the matter

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