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Paper: α-Elements Abundances in the Large Magellanic Cloud Bar
Volume: 458, Galactic Archaeology: Near-Field Cosmology and the Formation of the Milky Way
Page: 347
Authors: Van Swaelmen, M. d.; Hill, V.; Primas, F.
Abstract: We carried out a spectroscopy survey of about 110 stars located in the bar of the Large Magellanic Cloud (LMC) that combined with photometry already available allowed us to derive photometric temperatures, surface gravities, microturbulence velocity, overall metallicity, [Fe/H] and [α/Fe] ratios. We compare our results to Galactic stellar populations and to the LMC inner disc sample.
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