Galactic Outflows and the pollution of the Galactic Environment by Supernovae
E.M. de Gouveia Dal Pino, C. Melioli, A. D Ercole, F. Brighenti, A., Raga

TL;DR
This paper investigates how supernova explosions in star-forming galaxies create hot superbubbles that drive galactic fountains and winds, influencing halo clouds, gas recycling, and chemical enrichment.
Contribution
It provides 3D hydrodynamical simulations showing the formation of galactic fountains, their altitude limits, and implications for halo cloud formation and chemical distribution.
Findings
Fountains reach up to 5 kpc, forming intermediate-velocity clouds.
High-velocity clouds may form from intergalactic gas or magnetic fields.
Ejected material mostly falls back near the original region, affecting galaxy chemistry.
Abstract
We here explore the effects of the SN explosions into the environment of star-forming galaxies like the Milky Way. Successive randomly distributed and clustered SNe explosions cause the formation of hot superbubbles that drive either fountains or galactic winds above the galactic disk, depending on the amount and concentration of energy that is injected by the SNe. In a galactic fountain, the ejected gas is re-captured by the gravitational potential and falls back onto the disk. From 3D nonequilibrium radiative cooling hydrodynamical simulations of these fountains, we find that they may reach altitudes up to about 5 kpc in the halo and thus allow for the formation of the so called intermediate-velocity-clouds (IVCs) which are often observed in the halos of disk galaxies. The high-velocity-clouds that are also observed but at higher altitudes (of up to 12 kpc) require another mechanism…
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