Table 1: Characteristic quantities for the evolution of the 60 ${M}_\odot $ star (Z=0.02), adopted as input for our hydrodynamic simulations.
Phase End of phase [yr] $\Delta$t [yr] $\dot{m}$ [ ${M}_\odot~{\rm yr}^{-1}$] V [ ${\rm km}~ {\rm s}^{-1}$] $n_{{\rm photon}}$ [s-1]
Main Sequence 3.4499 $\times$ 106 3.4499 $\times$ 106 3.51 $\times$ 10-6 2420 7.12 $\times$ 1047
LBV 3.4796 $\times$ 106 2.9700 $\times$ 104 4.71 $\times$ 10-4 492 6.65 $\times$ 1047
Wolf-Rayet 3.8861 $\times$ 106 4.0650 $\times$ 105 6.41 $\times$ 10-5 2250 6.22 $\times$ 1049

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