The Gaia-ESO Survey: the first abundance determination of the pre-main-sequence cluster gamma Velorum
Context. Knowledge of the abundance distribution of star forming regions and young clusters is critical to investigate a variety of issues, from triggered star formation and chemical enrichment by nearby supernova explosions to the ability to form planetary systems. In spite of this, detailed abundance studies are currently available for relatively
Spina, L. et al.
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2014