Pre-supernova evolution, compact-object masses, and explosion properties of stripped binary stars

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Fig. 3.

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CO core masses M_CO at the core-helium exhaustion as a function of initial mass M_ini of our single stars and the Case A, B, and C stripped stars. Models leading to BHs and likely experiencing significant fallback are indicated (see Sects. 4.1 and 4.2 for more details).

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