\begin{table}%t1 %%\centering \par \caption {\label{tab1}Derived columns, areal coverages, and radial velocities (km~s$^{-1}$) inferred from UV resonance lines.} \begin{tabular}{crcrcrlrc} \hline\hline \noalign{\smallskip} N~V lines & ($\xi = 75$ km~s$^{-1}$)$\colon$ & & & & & & & \\ $T_{\rm disk}$ & Col. density & & Fractional & Area & Vel. & Vel. & $\tau_{\rm line}$ & $\tau_{\rm line}$ \\ & (Abs)~~~ & (Emis) & (Abs) & (Emis) & (Abs) & (Emis) & (Abs) & (Emis) \\ \hline 34~000 & $1.5\times10^{19}$ & -- & 1.0 & 0.0 & 0 & -- & 0.3 & -- \\ 34~000 & $1.5\times10^{19}$ & $5\times10^{18}$ & 0.4 & 0.4: & 0 & +75 & 0.3 & 0.1 \\ \par 28~000 & $3\times10^{21}$ & -- & 1.0 & 0.0 & 0 & -- & 0.6 & -- \\ 28~000 & $3\times10^{21}$ & $3\times10^{21}$ & 0.4 & 0.4: & 0 & +50 & $0.6$ & $0.6$ \\ \par \hline \par C~IV lines & ($\xi = 90$~km~s$^{-1}$)$\colon$ & & & & & & & \\ $T_{\rm disk}$ & Col. density & & Fractional & Area & Vel. & Vel. & $\tau_{\rm line}$ & $\tau_{\rm line}$ \\ & (Abs)~~~ & (Emis) & (Abs) & (Emis) & (Abs) & (Emis) & (Abs) & (Emis) \\ \hline \noalign{\smallskip} 24~000 & $3\times10^{21}$ & -- & 1.0 & 0.2 & 0 & -- & 15 & -- \\ 24~000 & $3\times10^{21}$ & $3\times10^{21}$ & 0.4 &0.8 & 0 & +125& 5 & 5 \\ \par 20~000 & $3.5\times10^{19}$ & -- & 1.0 & 0.0 & 0 & -- & 40 & -- \\ 20~000 & $1.7\times10^{17}$ & $1.7\times10^{17}$ & 0.4 & 1.0 & 0 & +125 & 0.2 & 0.2 \\ \hline Si~IV $\lambda$1403 & ($\xi = 75$)$\colon$ & & & & & & \\ $T_{\rm disk}$ & Col. density & & Fractional & Area & Vel. & Vel. & $\tau_{\rm line}$ & $\tau_{\rm line}$ \\ & (Abs)~~~ & (Emis) & (Abs) & (Emis) & (Abs) & (Emis) & (Abs) & (Emis) \\ \hline 22~000 & $5\times10^{18}$ & -- & 1.0 & 0.0 & 0 & -- & 2 & -- \\ 22~000 & $5\times10^{18}$ & $5\times10^{18}$ & 1.0 & 2.0 & +25 & +50 & 2 & 2 \\ \par 18~000 & $3\times10^{18}$ & -- & 1.0 & 0.0 & 0 & -- & 1.5 & -- \\ 18~000 & $3\times10^{18}$ & $3\times10^{18}$ & 1.0 & 6.5 & +25 & +50 & 1.5 & 1.5 \\ \hline \end{tabular} \end{table}