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Simulations of Merging Clusters of Galaxies

Published online by Cambridge University Press:  30 March 2016

Sabine Schindler
Sabine Schindler*
Affiliation:
Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Birkenhead CH41 1LD, U.K.

Abstract

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Numerical simulations of cluster mergers reveal many characteristics of the merging process: shock structure and strength, observational signatures of the dynamical state, effects on the mass determination, turbulence and the evolution of the X-ray luminosity and the magnetic field. In this article I review the results obtained from various simulations over the last years.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 12: Highlights of Astronomy. As presented at the XXIVth General Assembly of the IAU, 2000 , 2002 , pp. 531 - 533
Copyright
Copyright © Astronomical Society of Pacific 2002

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