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Table 2.

Mass-loss rate values applied in the synthetic spectra computations, compared to those that Hainich et al. (2015) would predict for the same stars.

Mini Label log h log r log Hainich
(M/yr) (M/yr) (M/yr)
20 T-1 (0.28) −8.48 −10.48 −10.77
20 T-2 (0.50) −7.80 −9.80 −10.39
20 T-3 (0.75) −6.89 −8.89 −8.68
20 T-4 (0.98) −5.77 −7.77 −7.99
20 T-5 (pMS) −5.50 −7.50 −8.17

59 T-5 (0.28) −7.00 −9.00 −9.29
59 T-6 (0.50) −6.70 −8.70 −8.29
59 T-7 (0.75) −5.82 −7.82 −7.52
59 T-8 (0.98) −4.92 −6.92 −7.00
59 T-10 (pMS) −4.70 −6.70 −7.50

131 T-11 (0.28) −6.17 −8.17 −8.53
131 T-12 (0.5) −5.89 −7.89 −8.04
131 T-13 (0.75) −4.96 −6.96 −9.10
131 T-14 (0.98) −4.27 −6.27 −7.80
131 T-15 (pMS) −4.23 −6.23 −7.27

Notes. log r means the reduced mass-loss rate, and log h the “higher”, i.e., the nominal rate as applied in the evolutionary sequences in Paper 1 (i.e., computed using our Eqs. (1) or (2)).

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