Quantifying Supernovae-Driven Multiphase Galactic Outflows
Miao Li, Greg L. Bryan, Jeremiah P. Ostriker

TL;DR
This study uses high-resolution 3D simulations to quantify how supernovae drive multiphase galactic outflows, revealing dependencies on gas surface density and physical processes affecting energy and metal ejection.
Contribution
It provides new quantitative insights into the mass, energy, and metal loading efficiencies of supernova-driven outflows across different galactic conditions.
Findings
Mass loading factor decreases with increasing gas surface density as $ ightarrow \, ext{eta}_m \, ext{proportional to} \, ext{Sigma}_{gas}^{-0.61}$.
Approximately 10-50 ext% of supernova energy and 40-80 ext% of metals are carried away by outflows.
Hot phase gas dominates energy and metal transport in the outflows.
Abstract
Galactic outflows are ubiquitously observed in star-forming disk galaxies and are critical for galaxy formation. Supernovae (SNe) play the key role in driving the outflows, but there is no consensus as to how much energy, mass and metal they can launch out of the disk. We perform 3D, high-resolution hydrodynamic simulations to study SNe-driven outflows from stratified media. Assuming SN rate scales with gas surface density as in the Kennicutt-Schmidt (KS) relation, we find the mass loading factor, , defined as the mass outflow flux divided by the star formation surface density, decreases with increasing as . Approximately 50 marks when 1. About 10-50\% of the energy and 40-80\% of the metals produced by SNe end up in the outflows.…
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