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Fig. 4


Typical pre-SN aspect of the CSM around a 15 M star (left panel) ending its stellar life as an RSG (and exploding as a type IIP SN), and around a 60 M star (right panel), ending as a WR star (exploding as a type Ibc SN). In each panel, we also show the mean density and temperature in the small window as a function of the radius.

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