More Pieces of the Puzzle: Chemistry and Substructures in the Galactic Thick Disk
We present a study of the chemical abundances of solar neighborhood stars associated with dynamical structures in the Milky Way's (thick) disk. These stars were identified as an overdensity in the eccentricity range 0.3 < ε < 0.5 in the Copenhagen-Geneva
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|Source:||Astrophysical Journal, The|
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