V_ϕ–V_Z diagram for stars with [Fe/H] > −1.4 in Nissen & Schuster (2010). V_ϕ is the Galactic rotational velocity component, V_ϕ = V_LSR + 232.8 km s⁻¹, and V_Z is the component perpendicular to the Galactic plane, V_Z = W_LSR. Stars from Nissen & Schuster (2010) belonging to the high-α sequence are shown with blue circles and those on the low-α sequence with filled red circles. G 112-43/44 is indicated with a black square. The three α-poor halo stars discussed in Sect. 4 are shown with asterisks. The green boxes indicate the location of the Helmi streams according to Koppelman et al. (2019b).