Speaker
Viola Hegedűs
Description
We will present new models simulating the chemical evolution of our Galaxy using abundances from MWM for which we are using the multi-zone chemical evolution environment OMEGA+. We compare the observed elemental abundance patterns of stars with the theoretical prediction of various evolution scenarios, such as the two-infall and parallel formations. We also undertook a comparison between APOGEE, GALAH and Gaia-ESO surveys to uncover the systematical differences between survey, which is essential to understand the effect of discrepancies on existing Milky Way chemical maps.
