Enhanced mass loss of very massive stars: Impact on the evolution, binary processes, and remnant mass spectrum

Open Access

Fig. 7.

Pre-SN mass (markers) and remnant mass (lines) as a function of the ZAMS mass for the three mass-loss rates, indicated by the marker style and color. The horizontal gray lines indicate different fates (PPISN, PISN, and DBH) based on the final He core mass.

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