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Table 5

Increase of mass-loss rates over the first bi-stability jump in non-rotating Galactic models using the Vink and the experimental wind scheme.

Vink wind Experimental wind

M [M] cool/hot cool/hot
20 14.5 5.0
30 14.0 4.5
40 13.8 4.1
60 13.4 3.9

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