\begin{table}%t1
\caption{\label{log1}Si{\sc iv} SEI model profile fitting parameters for the core sample.}
%\centering
\par
\begin{tabular}{llllllccc}
\hline \hline \noalign{\smallskip}
\multicolumn{1}{l}{Star}
&\multicolumn{1}{l}{Sp. type}
&\multicolumn{1}{l}{$T_{\rm eff}$ (kK)}
&\multicolumn{1}{l}{$v_\infty$}
&\multicolumn{1}{l}{$\beta$}
&\multicolumn{1}{l}{$v_{\rm turb}$}
&\multicolumn{1}{l}{$\tau_{\rm {rad}}(w)$(blue/red)}
&\multicolumn{1}{l}{$\langle$\Mdot~$q_i$$\rangle$(blue)}
&\multicolumn{1}{l}{$\langle$\Mdot~$q_i$$\rangle$(red)}
\\                                 
 & & & & & & &(10$^{-9}~M_\odot$ yr$^{-1}$) & (10$^{-9}~M_\odot$ yr$^{-1}$) \\
\hline
HD 13866    & B2 Ib-II:p  & 18.8 & 860  &   0.7  &  0.03 & 1.45 & 0.52 &  
0.70
\\
HD 14134    & B3 Ia & 16.5 & 495  &   0.5  &  0.10 & 1.37 & 0.83 &  1.39 
\\
HD 14143  &  B2 Ia  & 18.0  & 525  &   3.5  &  0.25 & 1.80 & 7.46 & 8.36 
\\
HD 36371    &  B4 Ib  & 16.5    &  465 &   0.8 &  0.17 & 1.10 & 0.38 &  
0.46 \\
HD 42087    &  B2.5 Ib  & 18.0 &  630 &    1.2 &  0.11 & 1.04 & 0.66 &  
1.24 \\
HD 43384    &  B3 Iab & 16.5 &  630 &    0.9 &  0.20 & 1.19 & 1.11 & 2.82 
\\
HD 47240  & B1 Ib  & 20.5 & 955  &   1.0  &  0.07 & 1.04 & 1.36 &  2.99 \\
HD 51309   & B3 Ib  & 16.5 &  730 &    0.5 &  0.15 & 1.55 & 0.94 &  1.81 
\\
HD 53138  & B3 Ia & 16.5 &  515 &    1.1 &  0.28 & 1.22 & 1.97 &  2.28 \\
HD 58350  & B5 Ia  & 15.0 &  380 &    0.8 &  0.25 & 2.04 & 0.90 & 1.25 \\
HD 58510    & B1 Ib-II & 20.5 & 915  &   0.9  &  0.19 & 1.79 & 1.37 & 1.62 
\\
HD 77581    & B0.5 Iae & 26.0  & 655  &   1.0  &  0.22 & 1.80 & 1.19 &  
1.72 \\
HD 79186    & B5 Ia & 15.0 & 435  &   0.8  &  0.23 & 1.73 & 0.86 &  1.09 
\\
HD 93827   & B1 Ib  & 20.5 & 590  &   0.5  &  0.16 & 1.64 & 0.10 & 0.15 \\
HD 111934    & B1.5 Ib & 18.5 & 935  &   3.1  &  0.15 & 1.46 & 4.62 &  
6.35 \\
HD 111973    & B3 Ia & 16.5 & 520  &   0.5  &  0.25 & 1.43 & 0.87 &  1.31 
\\
HD 111990   & B2 Ib & 18.0 & 715  &   3.3  &  0.12 & 1.97 & 2.14 &  2.50 
\\
HD 119608  & B1 Ib  & 20.5  & 925  &   0.6  &  0.25 & 1.14 & 2.05 & 3.69 
\\
HD 148379 & B2 Iap & 18.0 & 560  &   3.2  &  0.17 & 1.32 & 3.78 &  9.86 \\
HD 152236    & B0.5 Ia & 26.0 & 470  &   2.0  &  0.31 & 1.12 & 1.42 &  
2.03 \\
HD 152667    & B0 Ia & 27.5 & 800  &   2.5  &  0.28 & 1.78 & 4.44 &  4.81 
\\
HD 155985   & B0.7 Ib & 23.5 & 940  &   0.5  &  0.13 & 1.24 & 0.60 & 0.95 
\\   
HD 157246 & B1 Ib & 20.5 & 600  &   0.5  &  0.31 & 1.08 & 0.67 & 1.56 \\
HD 198478    & B2.5 Ia & 17.5 & 560  &   2.0  &  0.24 & 1.34 & 2.14 &  
4.16 \\
HD 225094    & B3 Ia & 16.5 & 485  &   0.5  &  0.21 & 1.75 & 0.81 & 0.78 \\
\hline
\end{tabular}
\tablefoot {$T_{\rm eff}$ from Searle et~al. (\cite{Sear08}). The $\langle$\Mdot~$q_i$$\rangle$~values include a few cases where~$\tau_{\rm {rad}}(w)$ exceeds~5.0 in isolated velocity bins.}
\vspace*{1mm}
\end{table}