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Table 2

Reformulation of the grid of wind solutions from KK17 (their Table 1), using their stellar parameters, but performing our own self-consistent solutions for the line-force and wind parameters.

Model Teff (K) log g R* (R) k α δ v (km s−1)
    Main sequence (V)
325−V 32.5 3.92 7.4 0.015 ± .001 0.672 ± .005 0.032 ± .001 3330±180 −8.222 ± .097 −0.855 −0.368
350−V 35.0 3.92 8.3 0.131 ± .006 0.607 ± .004 0.090 ± .002 2210±120 −6.783 ± .096 0.137 0.636
375−V 37.5 3.92 9.4 0.169 ± .010 0.524 ± .005 0.046 ± .002 1980±130 −6.816 ± .101 −0.293 0.143
400−V 40.0 3.92 10.7 0.162 ± .009 0.495 ± .006 0.015 ± .003 2040±130 −6.732 ± .095 −0.595 −0.130
425−V 42.5 3.92 12.2 0.136 ± .007 0.519 ± .005 0.013 ± .002 2310±130 −6.380 ± .090 −0.584 −0.034

    Giants (III)
300−III 30.0 3.49 13.1 0.048 ± .001 0.684 ± .002 0.102 ± .001 2070 ± 220 −6.789 ± .111 0.007 0.419
325−III 32.5 3.53 13.4 0.065 ± .002 0.680 ± .003 0.100 ± .001 2100±180 −6.385 ± .068 0.047 0.536
350−III 35.0 3.58 13.9 0.081 ± .003 0.661 ± .004 0.085 ± .002 2150±140 −6.111 ± .066 −0.014 0.509
375−III 37.5 3.63 14.4 0.092 ± .004 0.637 ± .005 0.068 ± .002 2190±140 −5.943 ± .070 −0.120 0.433
400−III 40.0 3.67 15.0 0.093 ± .004 0.615 ± .005 0.049 ± .002 2170±130 −5.858 ± .069 −0.238 0.152
425−III 42.5 3.72 15.6 0.091 ± .003 0.595 ± .004 0.031 ± .002 2220±130 −5.810 ± .060 −0.463 0.014

    Supergiants (I)
325−I 32.5 3.30 21.4 0.054± .002 0.689 ± .003 0.092 ± .002 1910±220 −5.887 ± .081 0.120 0.463
350−I 35.0 3.41 20.5 0.065 ± .002 0.674 ± .004 0.077 ± .002 2100±200 −5.732 ± .068 0.038 0.512
375−I 37.5 3.52 19.8 0.077 ± .003 0.657 ± .004 0.065 ± .002 2280 ±160 −5.606 ± .067 −0.174 0.315
400−I 40.0 3.63 19.1 0.084± .003 0.627 ± .004 0.046 ± .002 2430 ±140 −5.629 ± .067 −0.301 0.115
425−I 42.5 3.75 18.5 0.096 ± .004 0.573 ± .005 0.023 ± .002 2470±130 −5.779 ± .068 −0.527 −0.034

Notes. Differences in logarithm scale on mass-loss rate, compared with both formulae from Vink et al. (2001) and Krtička & Kubát (2017), are included in the last two columns (see also Fig. 5).

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