Mass transfer on a nuclear timescale in models of supergiant and ultra-luminous X-ray binaries

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Fig. 3.

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Mass–radius exponent of our initial 60 M_⊙ model in the same way as for the blue line in Fig. 2, but here for models where the internal helium gradient dY/dm has been artificially adjusted (see Sect. 2) to values indicated in the legend.

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