Fig. 3

Transformed mass-loss rates Ṁt (Eq. (24)) versus stellar temperatures T⋆ for our sample of putatively single WC (circles) and WO stars (squares). Filled symbols indicate objects in the Galaxy, empty symbols objects in the LMC. Some symbols have been shifted to avoid overlaps. The grey dashed line indicates the transformed mass-loss rate adopted for our artificial model sequence.
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