HIGHLIGHTS
- What: The authors aim to reproduce the observed MDF of the Galactic bulge by testing scenario in which the metal-poor component of the bulge is formed by stars formed in situ during strong burst of star formation while the population is formed by stars created in situ during second burst of star formation and/or stars accreted from the innermost part of the Galactic disk as an effect of growing bar. The aim of this work is to confirm (or disprove) this hypothesis by adopting a chemical evolution model that includes both multiple SF episodes and . . .
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