Same as Fig. 5 but only for systems with initial mass M= 1.5 and 2.0 M_⊙. The figures show models with two different values of B_wind (B_wind = 0 in red and B_wind = 10⁴ in green) and two different circularisation efficiencies (F_tide = 1 with filled symbols and F_tide = 0.01 with open symbols). Grey rectangles indicate initial orbital parameters, and the filled rectangles mark those systems that reached core-He burning when a tidally enhanced mass loss and a reduced tidal efficiency are combined (B_wind = 10⁴ and F_tide = 0.01).