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.
Luminosity class V

Model ${T_{\rm eff}}$ ${M_\star}\over{M_\odot}$ ${R_\star}\over{R_\odot}$ $\log g$ $\log\left({L_\star}\over{L_\odot}\right)$ $H_\star$ $\log\dot{M}$ $\beta$ $v_\infty$

(K) (cm s^-2) ( $10^{-4}~R_\star$ ) ( $M_{\odot }$ /yr) (km s^-1)

1V 48 618 68.9 12.3 4.094 5.882 8.308 -5.375 0.8 3240

2V 46 070 56.6 11.4 4.075 5.722 8.375 -5.599 0.8 3140

3V 43 511 45.2 10.7 4.032 5.568 8.971 -5.805 0.8 2950

4V 40 964 37.7 10.0 4.012 5.404 9.046 -6.072 0.8 2850

5V 38 406 30.8 9.3 3.987 5.229 9.314 -6.369 0.8 2720

6V 35 861 25.4 8.8 3.951 5.062 9.712 -6.674 0.8 2570

7V 33 306 21.2 8.3 3.924 4.883 9.934 -7.038 0.8 2450

8V 32 028 19.3 8.0 3.915 4.783 9.988 -7.252 0.8 2400

9V 30 820 17.7 7.8 3.897 4.697 10.16 -7.445 0.8 2330

10V 28 270 14.8 7.4 3.864 4.502 10.40 -7.913 0.8 2210

Luminosity class III

1III 48 132 82.8 15.1 3.996 6.042 9.098 -5.125 1.0 3080

2III 45 363 68.4 15.0 3.919 5.934 10.04 -5.239 1.0 2850

3III 42 595 56.6 14.8 3.848 5.813 10.82 -5.397 1.0 2660

4III 39 815 47.4 14.7 3.777 5.690 11.53 -5.585 1.0 2490

5III 37 049 39.0 14.7 3.692 5.564 12.63 -5.791 1.0 2290

6III 34 282 32.6 14.7 3.614 5.430 13.50 -6.051 1.0 2130

7III 31 504 27.4 14.7 3.539 5.283 14.20 -6.377 1.0 1990

8III 30 127 25.1 14.8 3.495 5.211 14.69 -6.551 1.0 1920

9III 28 781 23.5 14.8 3.464 5.134 14.73 -6.758 1.0 1870

10III 26 011 20.2 15.0 3.386 4.970 15.18 -7.230 1.0 1750

Luminosity class Ia

1Ia 47 641 104.7 55.9 18.6 3.916 3.639 6.206 9.502 -4.896 1.0 3000

2Ia 44 642 86.5 48.6 19.6 3.788 3.533 6.139 11.63 -4.922 1.0 2620

3Ia 41 651 74.7 42.5 20.6 3.681 3.431 6.062 12.95 -5.014 1.0 2400

4Ia 38 663 64.3 37.4 21.8 3.566 3.327 5.981 14.44 -5.134 1.0 2190

5Ia 35 673 54.8 33.1 23.1 3.446 3.223 5.892 16.15 -5.295 1.0 1990

6Ia 32 687 46.7 29.5 24.6 3.322 3.120 5.795 17.90 -5.509 1.0 1810

7Ia 31 194 43.1 27.9 25.4 3.260 3.068 5.741 18.70 -5.644 1.0 1730

8Ia 29 719 40.9 26.0 26.2 3.211 3.012 5.683 18.67 -5.815 1.0 1690

9Ia 26 731 36.1 23.7 28.1 3.094 2.909 5.563 19.35 -6.202 1.0 1570

10Ia 23 733 32.4 22.0 30.5 2.976 2.805 5.427 19.53 -5.409 1.0 740

**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.
Luminosity class V
Model	${T_{\rm eff}}$	${M_\star}\over{M_\odot}$	${R_\star}\over{R_\odot}$	$\log g$	$\log\left({L_\star}\over{L_\odot}\right)$	$H_\star$	$\log\dot{M}$	$\beta$	$v_\infty$
	(K)			(cm s^-2)		( $10^{-4}~R_\star$ )	( $M_{\odot }$ /yr)		(km s^-1)
1V	48 618	68.9	12.3	4.094	5.882	8.308	-5.375	0.8	3240
2V	46 070	56.6	11.4	4.075	5.722	8.375	-5.599	0.8	3140
3V	43 511	45.2	10.7	4.032	5.568	8.971	-5.805	0.8	2950
4V	40 964	37.7	10.0	4.012	5.404	9.046	-6.072	0.8	2850
5V	38 406	30.8	9.3	3.987	5.229	9.314	-6.369	0.8	2720
6V	35 861	25.4	8.8	3.951	5.062	9.712	-6.674	0.8	2570
7V	33 306	21.2	8.3	3.924	4.883	9.934	-7.038	0.8	2450
8V	32 028	19.3	8.0	3.915	4.783	9.988	-7.252	0.8	2400
9V	30 820	17.7	7.8	3.897	4.697	10.16	-7.445	0.8	2330
10V	28 270	14.8	7.4	3.864	4.502	10.40	-7.913	0.8	2210
Luminosity class III
1III	48 132	82.8	15.1	3.996	6.042	9.098	-5.125	1.0	3080
2III	45 363	68.4	15.0	3.919	5.934	10.04	-5.239	1.0	2850
3III	42 595	56.6	14.8	3.848	5.813	10.82	-5.397	1.0	2660
4III	39 815	47.4	14.7	3.777	5.690	11.53	-5.585	1.0	2490
5III	37 049	39.0	14.7	3.692	5.564	12.63	-5.791	1.0	2290
6III	34 282	32.6	14.7	3.614	5.430	13.50	-6.051	1.0	2130
7III	31 504	27.4	14.7	3.539	5.283	14.20	-6.377	1.0	1990
8III	30 127	25.1	14.8	3.495	5.211	14.69	-6.551	1.0	1920
9III	28 781	23.5	14.8	3.464	5.134	14.73	-6.758	1.0	1870
10III	26 011	20.2	15.0	3.386	4.970	15.18	-7.230	1.0	1750
Luminosity class Ia
1Ia	47 641	104.7 55.9	18.6	3.916 3.639	6.206	9.502	-4.896	1.0	3000
2Ia	44 642	86.5 48.6	19.6	3.788 3.533	6.139	11.63	-4.922	1.0	2620
3Ia	41 651	74.7 42.5	20.6	3.681 3.431	6.062	12.95	-5.014	1.0	2400
4Ia	38 663	64.3 37.4	21.8	3.566 3.327	5.981	14.44	-5.134	1.0	2190
5Ia	35 673	54.8 33.1	23.1	3.446 3.223	5.892	16.15	-5.295	1.0	1990
6Ia	32 687	46.7 29.5	24.6	3.322 3.120	5.795	17.90	-5.509	1.0	1810
7Ia	31 194	43.1 27.9	25.4	3.260 3.068	5.741	18.70	-5.644	1.0	1730
8Ia	29 719	40.9 26.0	26.2	3.211 3.012	5.683	18.67	-5.815	1.0	1690
9Ia	26 731	36.1 23.7	28.1	3.094 2.909	5.563	19.35	-6.202	1.0	1570
10Ia	23 733	32.4 22.0	30.5	2.976 2.805	5.427	19.53	-5.409	1.0	740

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