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Fig. 2


Evolution of the eccentricity (top) and orbital period (bottom, in days) for the enhanced-wind models as a function of the donor’s mass. The curves correspond to different initial orbital periods: 30 (solid, black), 100 (red, dotted), 200 (green, short-dashed) days, 1 (blue, long-dashed), 1.5 (cyan, dot-short dashed) and 2 years (magenta, dot-long dashed). The initial stellar masses are 1.2 + 1.0 M.

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