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Paper: |
Observational Properties of the Chemically Divided Galactic Disks |
Volume: |
458, Galactic Archaeology: Near-Field Cosmology and the Formation of the Milky Way |
Page: |
229 |
Authors: |
Lee, Y. S.; Beers, T. C.; An, D.; the SEGUE Collaboration |
Abstract: |
We make use of [α/Fe] ratios derived from the spectra of 17,277
SEGUE G dwarfs to separate them into likely thin- and thick-disk
subsamples, and investigate the rotational velocity and eccentricity
gradients with metallicity, [Fe/H], distance from the plane, |Z|, and
Galactocentric distance, R, in order to provide observational constraints
on contemporary models of the formation of the Milky Way's thick disk. |
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