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Fig. 25.

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Vϕ distribution for each cell defined in Fig. 20. The value of the dispersion in Vϕ is also shown for each cell. Thick disc stars with Vϕ ∼ 140 km s−1 are seen in panels H and E where there is less contamination by thin disc stars (with Vϕ around 200 km s−1 – cells G and D) and the spheroidal component (with Vϕ around 80 km s−1 cells I, F, and C). A counter-rotating tail is noticeable in cell C.

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