Fig. C.1.
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Vϕ distribution for metal-poor stars confined to 3 kpc from the Galactic plane. (a) Vϕ distribution for the metal-poor ([Fe/H]≤-1.0) set — full subset in yellow and the low-eccentricity stars in blue. Ratio of prograde (Vϕ> 50 km s−1) to retrograde (Vϕ< -50 km s−1) stars is also shown. (b) Same as above but for the very metal-poor ([Fe/H]≤-1.5) subset. The prograde to retrograde ratio is provided for each subsample.
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