Fig. A.1
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Time evolution of stellar wind masses of different temperatures for the low (dashed) and high (dotted) resolution models: Panel a: Mass of cool (T < 104 K) material vs time enclosed within spheres of 0.5 pc (blue) and 3.0 pc (purple). Panel b: Idem for hot (T > 104 K) material. Panel c: Plot of material with T > 104 K (blue) and T > 105 K (purple) enclosed within spheres of 0.5 pc (blue) and 3.0 pc (purple). Panel d: Ratio of cool (T < 104 K) to hot (T > 104 K) material.
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