Gaseous infall triggering starbursts in simulated dwarf galaxies
Abstract
Using computer simulations, we explored gaseous infall as a possible explanation for the starburst phase in Blue Compact Dwarf galaxies. We simulate a cloud impact by merging a spherical gas cloud into an isolated dwarf galaxy. We investigated which conditions were favourable for triggering a burst and found that the orbit and the mass of the gas cloud play an important role. We discuss the metallicity, the kinematical properties, the internal dynamics and the gas, stellar and dark matter distribution of the simulations during a starburst. We find that these are in good agreement with observations and depending on the set-up (e.g. rotation of the host galaxy, radius of the gas cloud), our bursting galaxies can have qualitatively very different properties. Our simulations offer insight in how starbursts start and evolve. Based on this, we propose what postburst dwarf galaxies will look like.
Cite
@article{arxiv.1405.2339,
title = {Gaseous infall triggering starbursts in simulated dwarf galaxies},
author = {Robbert Verbeke and Sven De Rijcke and Mina Koleva and Annelies Cloet-Osselaer and Bert Vandenbroucke and Joeri Schroyen},
journal= {arXiv preprint arXiv:1405.2339},
year = {2015}
}
Comments
Accepted for publication in MNRAS | 16 pages, 16 figures