Further diagrams of the publication Schürmann, Xu, et al. (Astronomy & Astrophysics)

Same as Fig. 3, but for initial donor masses of 8, 9, 10, 12, 15, 20, 25, 30, 40, 50, 70 and 99 Msol (see file name).

Evolutionary outcome of our binary models at the time when the first SR has formed, or when the system merges, as a function of initial orbital period P and initial mass ratio q, for six different mass-transfer efficiencies ε. Each black dot represents one model system, and their total number in each plot is 104. We coloured the plane according to the result of the closest model (Voronoi diagram). We mark the boundary between RLO Case A and B by a black line. The occurrence of a later RLO with a HeS donor (i.e. Case BB or BC) is indicated by pink hatches. If the companion to a SR is not a MS star but a post-MS star, we mark it by orange cross-hatches in case it is H-rich (BSG/RSG), or by pink cross-hatches if it is H-poor (HeS). White regions are those with no RLO (top) or RLO at ZAMS (bottom). In grey areas, the outcome is not none of the above (often two SN immediately after each other due to the final temporal resolution).