Constraining gas metal mixing strength in simulations using observations of the Milky Way's disc
This work explores the mixing rate of metals in the interstellar medium (ISM), comparing observational constraints from our solar neighbourhood to high resolution cosmological hydrodynamical simulations of Milky Way (MW)-like galaxies. The mixing rate, described by the coefficient C, is varied in simulations between 0 and 0.05, with resultant
Sarrato-Alós, J. et al.
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10
2023