The model of a radial minor merger proposed by [Quinn, ApJ 279, 596 (1984)], which successfully reproduces the observed regular shell systems in shell galaxies, is ideal for a test-particle simulation. We compare such a simulation with a self-consistent one. They agree very well in positions of the first generation of shells but potentially important effects - dynamical friction and gradual decay of the dwarf galaxy - are not present in the test-particle model, therefore we look for a proper way to include them. © Springer-Verlag Berlin Heidelberg 2011.
CITATION STYLE
Ebrová, I., Bartošková, K., Jungwiert, B., Jílková, L., & Křížek, M. (2011). Comparing various approaches to simulating the formation of shell galaxies. In Astrophysics and Space Science Proceedings (pp. 199–201). Kluwer Academic Publishers. https://doi.org/10.1007/978-3-642-20285-8_40
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