Abstract
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.
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© 1983 IAU
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White, S.D.M. (1983). Simulations of Galaxy Mergers. In: Athanassoula, E. (eds) Internal Kinematics and Dynamics of Galaxies. International Astronomical Union/Union Astronomique Internationale, vol 100. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7075-5_93
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DOI: https://doi.org/10.1007/978-94-009-7075-5_93
Publisher Name: Springer, Dordrecht
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