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Fig. 2.

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Evolution during different phases. Top: Indicative tracks of equal timesteps of 1kyr in the HRD with Y23 (left) and J88 (right), depicting the definition of each evolutionary phase. The initial mass is mentioned at the beginning of each track. The HD limit, where LBV-type winds kick in is also shown (grey dot-dashed line). Middle: Part of the stellar mass lost in each evolutionary phase, as a function of initial mass (evolution goes from top to bottom). We also show the value of the final helium core mass as a function of the initial (purple dotted line). Bottom: Fractional time spent in each evolutionary phase after the end of MS, as a function of initial mass (evolution goes from top to bottom).

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