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- W2032816401 abstract "Context. A previous study of F and G main-sequence stars in the solar neighborhood has revealed the existence of two distinct halo populations with a clear separation in [α/Fe] for the metallicity range −1.4 < [Fe/H] < −0.7. Taking into account the kinematics and ages of the stars, some Galactic formation models suggest that the “high-alpha” halo stars were formed in situ, whereas the “low-alpha” stars have been accreted from satellite galaxies." @default.
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- W2032816401 date "2012-06-22" @default.
- W2032816401 modified "2023-10-02" @default.
- W2032816401 title "Two distinct halo populations in the solar neighborhood" @default.
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- W2032816401 doi "https://doi.org/10.1051/0004-6361/201219342" @default.
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