Gaseous infall triggering starbursts in simulated dwarf galaxies

TL;DR

This study uses simulations to investigate how gaseous infall can trigger starbursts in dwarf galaxies, revealing the importance of cloud orbit and mass, and aligning results with observed properties.

Contribution

It introduces a simulation framework for gaseous infall triggering starbursts, highlighting the roles of cloud orbit and mass, and predicts postburst dwarf galaxy features.

Findings

Gas cloud orbit and mass influence starburst initiation.

Simulated properties match observed dwarf galaxy characteristics.

Different initial conditions lead to diverse galaxy properties.

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.