Chemo-orbital evidence from SDSS/SEGUE G-type dwarf stars for a mixed origin of the Milky Way's thick disk

Details Chemo-orbital evidence from SDSS/SEGUE G-type dwarf stars for a mixed origin of the Milky Way's thick disk Chemo-orbital evidence from SDSS/SEGUE G-type dwarf stars for a mixed origin of the Milky Way's thick disk

2012-01-08

arxiv.org/abs/1201.1635v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

13 pages, 9 figures, submitted to MNRAS

Scientific paper

We combine the estimated metallicities [Fe/H], abundances [\alpha/Fe], positions and motions of a sample of 27,500 local (7

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