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Fig. 1
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Ratio of accretion onto the secondary and primary stars, λ = ṁs/ ṁp, plotted against the binary mass ratio, qb = ms/mp. The data are merged from Siwek et al. (2023) for qb > 0.1 and from Eq. (10) which is adapted from Kelley et al. (2019). The plot extends towards qb = 0 but is truncated for clarity.
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