Mass-loading of outflows from evolving young massive clusters

Open Access

Fig. A.2.

Time evolution of L_mech (upper panel) and ${\bar{V}}_{cl}$ $\bar{V}_{\mathrm{cl}}$ (lower panel) for Z_MW, assuming the base prescription for all stars (solid blue), the base prescription for only WR stars (dashed blue), the Sander prescription with a T_eff dependence for WR stars with T_eff > 90 kK (dashed orange), and the Sander prescription without a T_eff dependence for all WR stars (dashed green).

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