Fig. 4.
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R2/RL filling factor for a system formed by a solar composition donor star of 1 M⊙, a NS of 1.4 M⊙ with Pinic, i = 1 d. We considered moderate IFB assuming αirr = 0.10. Blue lines represent detached conditions whereas black lines depict stages with a mass transfer rate Ṁ ≥ 10−11 M⊙ yr−1. IFB-driven pulsed mass transfer and HSBD occur in the model.
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