{ "id": "1903.03647", "version": "v1", "published": "2019-03-08T19:57:02.000Z", "updated": "2019-03-08T19:57:02.000Z", "title": "Variations of the stellar Initial Mass Function in Semi-Analytic Models: implications for the mass assembly of galaxies in the GAEA model", "authors": [ "Fabio Fontanot" ], "comment": "4 Pages, 2 Figures, Proceedings of IAU symposium 341, \"PanModel2018: Challenges in Panchromatic Galaxy Modelling with Next Generation Facilities\", Osaka, Japan", "categories": [ "astro-ph.GA" ], "abstract": "A wealth of observations recently challenged the notion of a universal stellar initial mass function (IMF) by showing evidences in favour of a variability of this statistical indicator as a function of galaxy properties. I present predictions from the semi-analytic model GAEA (GAlaxy Evolution and Assembly), which features (a) a detailed treatment of chemical enrichment, (b) an improved stellar feedback scheme, and (c) implements theoretical prescriptions for IMF variations. Our variable IMF realizations predict intrinsic stellar masses and mass-to-light ratios larger than those estimated from synthetic photometry assuming a universal IMF. This provides a self-consistent interpretation for the observed mismatch between photometrically inferred stellar masses of local early-type galaxies and those derived by dynamical and spectroscopic studies. At higher redshifts, the assumption of a variable IMF has a deep impact on our ability to reconstruct the evolution of the galaxy stellar mass function and the star formation history of galaxies.", "revisions": [ { "version": "v1", "updated": "2019-03-08T19:57:02.000Z" } ], "analyses": { "keywords": [ "stellar initial mass function", "semi-analytic model", "predict intrinsic stellar masses", "gaea model", "imf realizations predict intrinsic" ], "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable" } } }