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