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Fig. 6

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a) Evolution of αself as a function of time, tself, since the start of self-accretion for a 5 + 3 M system, with an initial orbital period, Pi of 3 d (dotted red curve), 7 d (solid black), 10 d (green short dashed) and 13 d (blue long-dashed). b) Evolution of the orbital period, Porb, as a function of q = M1/M2, for different initial orbital periods: 3 d (dot-dashed); 7 d (solid); 10 d (short-dashed) and 13 d (dotted). Black curves refer to classical calculations, and the red lines to the osculating scheme.

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