Similar to Fig. 6, but the rectangles representing the binary models are colored according to the integrated duration of a postinteraction detachment phase during which the core-He burning mass loser remains on the cooler side of the ZAMS line in the HR diagram. Rectangles corresponding to models with post-MS donors (either at the Hertzprung gap or the core-He burning stage, see the background colors) that are colored in various shades of green and yellow are models that produce partially stripped long-lived stars (see Sec. 3.4 and Sec. 5.4 for a discussion of this population).