A quantitative demonstration that stellar feedback locally regulates galaxy growth
arXiv:2009.08992 · doi:10.1093/mnras/staa2906
Abstract
We have applied stellar population synthesis to 500 pc sized regions in a sample of 102 galaxy discs observed with the MUSE spectrograph. We derived the star formation history and analyse specifically the "recent" () and "past" () age bins. Using a star formation self-regulator model we can derive local mass-loading factors, for specific regions, and find that this factor depends on the local stellar mass surface density, , in agreement with the predictions form hydrodynamical simulations including supernova feedback. We integrate the local - relation using the stellar mass surface density profiles from the Spitzer Survey of Stellar Structure in Galaxies (S4G) to derive global mass-loading factors, , as a function of stellar mass, . The - relation found is in very good agreement with hydrodynamical cosmological zoom-in galaxy simulations. The method developed here offers a powerful way of testing different implementations of stellar feedback, to check on how realistic are their predictions.
Accepted for publication in MNRAS
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