The triggering of starbursts in low-mass galaxies

TL;DR

This study analyzes the HI gas distribution and kinematics in 18 nearby starburst dwarf galaxies, revealing external interactions or gas infall as triggers for starbursts, with morphological evidence supporting these mechanisms.

Contribution

It provides the first detailed comparison of HI morphology in starburst and typical dwarf galaxies, linking asymmetries to external triggering mechanisms.

Findings

Starburst dwarfs show more asymmetric HI morphologies than typical irregulars.

Older starbursts have more symmetric HI distributions, indicating relaxation over time.

Most starburst dwarfs have potential external perturbers within 200 kpc.

Abstract

Strong bursts of star formation in galaxies may be triggered either by internal or external mechanisms. We study the distribution and kinematics of the HI gas in the outer regions of 18 nearby starburst dwarf galaxies, that have accurate star-formation histories from HST observations of resolved stellar populations. We find that starburst dwarfs show a variety of HI morphologies, ranging from heavily disturbed HI distributions with major asymmetries, long filaments, and/or HI-stellar offsets, to lopsided HI distributions with minor asymmetries. We quantify the outer HI asymmetry for both our sample and a control sample of typical dwarf irregulars. Starburst dwarfs have more asymmetric outer HI morphologies than typical irregulars, suggesting that some external mechanism triggered the starburst. Moreover, galaxies hosting an old burst (>100 Myr) have more symmetric HI morphologies than galaxies hosting a young one (<100 Myr), indicating that the former ones probably had enough time to regularize their outer HI distribution since the onset of the burst. We also investigate the nearby environment of these starburst dwarfs and find that most of them ($\sim$80$\%$) have at least one potential perturber at a projected distance <200 kpc. Our results suggest that the starburst is triggered either by past interactions/mergers between gas-rich dwarfs or by direct gas infall from the IGM.