SPAGNA, AlessandroAlessandroSPAGNACURIR, AnnaAnnaCURIRGIAMMARIA, MARCOMARCOGIAMMARIALATTANZI, Mario GilbertoMario GilbertoLATTANZIMURANTE, GiuseppeGiuseppeMURANTERE FIORENTIN, PaolaPaolaRE FIORENTIN2020-11-062020-11-06201897811071700871743-9213http://hdl.handle.net/20.500.12386/28202We have investigated the chemo-dynamical evolution of a Milky Way-like disk galaxy, AqC4, produced by a cosmological simulation integrating a sub-resolution ISM model. We evidence a global inside-out and upside-down disk evolution, that is consistent with a scenario where the ``thin disk'' stars are formed from the accreted gas close to the galactic plane, while the older ``thick disk'' stars are originated in situ at higher heights. Also, the bar appears the most effective heating mechanism in the inner disk. Finally, no significant metallicity-rotation correlation has been observed, in spite of the presence of a negative [Fe/H] radial gradient.STAMPAenConference paper10.1017/S1743921317006019000454738700070https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/chemodynamical-signatures-in-simulated-milky-waylike-galaxies/3DA716984D646CB6F9511BAE936532EA2018IAUS..330..263SFIS/05 - ASTRONOMIA E ASTROFISICA