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Fig. 11.

image

Tracks in Mbol vs. Log plane for BSG stages, using both a modified and unmodified bolometric magnitude due to the presence of the secondary. Grey tracks are original tracks with unmodified Mbol (as in Fig. 3). Blue, green and red tracks correspond to the first, second and third BSG stages with modified Mbol calculated by combining the V band flux of the primary and secondary and applying the bolometric correction (BC) based on the log g and Teff of the primary. Maroon tracks use a modified Mbol calculated by computing the bolometric magnitude for the sum of the luminosities of the primary and secondary. Top panel: close-up track of the 15 M model to more clearly illustrate the changes in the modified tracks. Bottom panel: models with initial masses of 12, 15, 20 and 30 M, mass ratio of q = 0.9 and initial period of log(P/days) = 3.0.

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