In-N-Out: the gas cycle from dwarfs to spiral galaxies
Charlotte R. Christensen, Romeel Dav\'e, Fabio Governato, Andrew, Pontzen, Alyson Brooks, Ferah Munshi, Thomas Quinn, James Wadsley

TL;DR
This study uses high-resolution galaxy simulations to analyze how galactic outflows and recycling influence star formation and angular momentum across a wide range of galaxy masses, aligning with observed galaxy properties.
Contribution
It provides a detailed quantification of outflow scalings, recycling timescales, and their effects on galaxy evolution, supported by a large suite of cosmological simulations.
Findings
Mass loading factor scales as v_circ^(-2.2)
Recycling occurs in about half of the outflow mass
Recycling timescale is approximately 1 Gyr, independent of halo mass
Abstract
We examine the scalings of galactic outflows with halo mass across a suite of twenty high-resolution cosmological zoom galaxy simulations covering halo masses from 10^9.5 - 10^12 M_sun. These simulations self-consistently generate outflows from the available supernova energy in a manner that successfully reproduces key galaxy observables including the stellar mass-halo mass, Tully-Fisher, and mass-metallicity relations. We quantify the importance of ejective feedback to setting the stellar mass relative to the efficiency of gas accretion and star formation. Ejective feedback is increasingly important as galaxy mass decreases; we find an effective mass loading factor that scales as v_circ^(-2.2), with an amplitude and shape that is invariant with redshift. These scalings are consistent with analytic models for energy-driven wind, based solely on the halo potential. Recycling is common:…
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