All Tables

Table 1: Stellar and wind parameters of our model grid. For supergiants, we list ${\log~g}$ values derived for both the spectroscopic and evolutionary mass. Values of ${T_{\rm eff}}$ and $R_\star$ for supergiants correspond to models with evolutionary masses. Adopted abundances by mass fraction are from Cox (2000): H = 0.7023, He = 0.2820, and, in units of 10^-3, C = 3.050, N = 1.100, O = 9.540, Si = 0.699, Fe = 1.360.
Table 2: Identification of the lines used in this study.