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Fig. 7.

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Stacked-bar chart showing how much of the primary star’s initial mass of 12.6 M is left at core collapse (red), and how much is lost (white hatching), as a function of the initial binary orbital period for our systems with an initial mass ratio of qi = 0.95. The helium core mass (red filling, black dots) is distinguished from the mass of the remaining H-rich envelope (red filling, no hatching) with a black line. The three colored white-hatched bars represent the mass lost via wind (azure), Case B RLOF (blue), and Case C RLOF (green).

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