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- W4242534015 abstract "Away from the young disk, several classes of early type stars are found. They include (i) the old, metal-poor blue horizontal branch stars of the halo and the metal-poor tail of the thick disk; (ii) metal-rich young A stars in a rapidly rotating subsystem but with a much higher velocity dispersion than the A stars of the young disk, and (iii) a newly discovered class of metal-poor young main sequence A stars in a subsystem of intermediate galactic rotation (V rot ≈ 120 km s −1 ). The existence and kinematics of these various classes of early type stars provide insight into the formation of the metal-poor stellar halo of the Galaxy and into the continuing accretion events suffered by our Galaxy." @default.
- W4242534015 created "2022-05-12" @default.
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- W4242534015 date "1995-01-01" @default.
- W4242534015 modified "2023-09-25" @default.
- W4242534015 title "Early-Type Stars" @default.
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- W4242534015 doi "https://doi.org/10.1017/s0074180900108484" @default.
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