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Fig. 16.

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Maximum BH and SN ejecta mass of single stars and accretors with facc ≤ 1.0 and facc ≤ 2.0 as a function of the maximum time spent in the LBV region of the HR diagram. The grey-shaded region indicates models for which we expect significant LBV-like mass loss such that the maximum BH and SN ejecta masses should be considered upper limits.

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