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Simulations of Galaxy Mergers

Published online by Cambridge University Press:  04 August 2017

Simon D. M. White*
Affiliation:
Department of Astronomy and Space Sciences Laboratory, University of California, Berkeley, CA 94720, U.S.A.

Abstract

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The last few years have seen a considerable amount of effort devoted to the problem of simulating the coalescence of galaxies. After a discussion of the merits and limitations of the N-body techniques that have been used, I summarise the insight this research gives into the mechanisms driving strong interactions in galaxy collisions and into the structure of the remnants such collisions produce.

Type
VI. Mergers
Copyright
Copyright © Reidel 1983 

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