Abundances of Main-Sequence Stars in the Hyades and the Pleiades
Carlos Allende Prieto (University of Texas)
David Yong (University of Texas)
David L. Lambert (University of Texas)
Open clusters, in particular those nearby, have always been very valuable to inspire and test theories of structure, formation, evolution, and nucleosynthesis in stars. We revisit the chemical abundances along the main sequence of the Hyades and the Pleiades with improved data and analysis techniques.
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