Simulating galactic outflows with kinetic supernova feedback

TL;DR

This paper introduces a kinetic supernova feedback model in cosmological simulations, demonstrating how pressure forces influence galactic outflows and morphology, with implications for galaxy evolution modeling.

Contribution

A new sub-grid kinetic feedback recipe for star formation in cosmological simulations that accounts for pressure forces affecting galactic outflows and morphology.

Findings

Pressure forces significantly alter outflow structures.

Galactic morphology is affected by feedback-driven superbubbles.

Mass loading of winds varies with galaxy mass.

Abstract

Feedback from star formation is thought to play a key role in the formation and evolution of galaxies, but its implementation in cosmological simulations is currently hampered by a lack of numerical resolution. We present and test a sub-grid recipe to model feedback from massive stars in cosmological smoothed particle hydrodynamics simulations. The energy is distributed in kinetic form among the gas particles surrounding recently formed stars. The impact of the feedback is studied using a suite of high-resolution simulations of isolated disc galaxies embedded in dark halos with total mass 10^{10} and 10^{12} Msol/h. We focus in particular on the effect of pressure forces on wind particles within the disc, which we turn off temporarily in some of our runs to mimic a recipe that has been widely used in the literature. We find that this popular recipe gives dramatically different results because (ram) pressure forces on expanding superbubbles determine both the structure of the disc and the development of large-scale outflows. Pressure forces exerted by expanding superbubbles puff up the disc, giving the dwarf galaxy an irregular morphology and creating a galactic fountain in the massive galaxy. Hydrodynamic drag within the disc results in a strong increase of the effective mass loading of the wind for the dwarf galaxy, but quenches much of the outflow in the case of the high-mass galaxy.