Comparing Various Approaches to Simulating the Formation of Shell Galaxies
| Autoři | |
|---|---|
| Rok publikování | 2011 |
| Druh | Článek ve sborníku |
| Konference | ENVIRONMENT AND THE FORMATION OF GALAXIES: 30 YEARS LATER: PROCEEDINGS OF SYMPOSIUM 2 OF JENAM 2010 |
| Fakulta / Pracoviště MU | |
| Citace | |
| Doi | http://dx.doi.org/10.1007/978-3-642-20285-8_40 |
| Obor | Astronomie a nebeská mechanika, astrofyzika |
| Klíčová slova | galaxies: interactions; galaxies: N-body simulations; galaxies: shell galaxies |
| Popis | 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. |
| Související projekty: |