\begin{table}%T1
\caption{\label{tab:StelPar}Stellar and wind parameters of our model grid.  For
supergiants, we list \logg\ values derived for both the spectroscopic
and evolutionary mass. Values of \teff\ and $R_\star$ for supergiants
correspond to models with evolutionary masses. Adopted abundances by
mass fraction are from Cox (\cite{Cox2000}): 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.}
  %\centering
\par
  \begin{tabular}{cccccccccc}
   \hline
  \hline
  \multicolumn{10}{c}{Luminosity class V}\\
    \hline
  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$^{-1}$) \\
  \hline
  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 \\
  \hline
   \multicolumn{10}{c}{Luminosity class III}\\
    \hline
  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 \\
  \hline
    \multicolumn{10}{c}{Luminosity class Ia}\\
  \hline
    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 \\
  \hline
\end{tabular}
\end{table}