Orbital properties of WR–COs and Cyg X-3 at the beginning (left) and end (right) of the WR–CO phase. We highlight the properties of WR–COs (triangular markers) and Cyg X-3-like binaries (non-triangular markers) that are BCO progenitors, comparing them to the properties of the whole sample of WR–COs (gray areas in the background). We distinguish binaries ending up as BBHs (purple upward triangles; red circles), as BNSs (gold downward triangles; yellow thin diamonds), or as BHNSs, either forming the BH (green rightward triangles; thick turquoise diamonds) or the NS first (blue leftward triangles; turquoise pentagons). The black rectangular box indicates the region of orbital parameters that we use to select Cyg X-3 candidates (Section 3.4). Black diagonal lines indicate orbital periods of 1 hour, 1 day or 1 year. Here we show the set evolved with α_CE = 3, Z = 0.02, G20 natal kick model and compactness CCSN model. In Figure 8 we show the same set, but with the delayed CCSN model.