\begin{table}%t4
%\centering
\par
\caption{Results from emission line measurements. H~{\sc i}  measurements are performed on the difference spectrum  (see text and Fig.~\ref{HI_spectrum}). The H~{\sc i} component at $14.5~\kms $ is not detected in absorption and is probably due to background gas situated behind the star HD~102065.} \label{Tab_emission}
\begin{tabular}{lccccc}
\hline\hline\noalign{\smallskip}
Species&
$ V_{\rm LSR}~({\rm {km~ s}^{-1}}) $& $ T_{\rm b}~{\rm (K)}$& $FWHM~~({\rm {km~ s}^{-1}})$&
$b~~({\rm {km~ s}^{-1}})$& $ N~~({\rm {cm}^{-2}})$\\
\hline\noalign{\smallskip}
H~{\sc i} ~ 21~cm difference)&$14.5\pm0.6$&$0.9\pm0.15$&$7.3\pm1.4$&$4.4\pm0.8$&$1.3\pm0.2\times 10^{19}$\\
&$4.2\pm0.1$   &$20.4\pm1.1$ &$3.2\pm0.2$ &$1.9\pm0.1$ &$1.3\pm0.07\times 10^{20}$\\
&$0.1\pm0.1$   &$13.4\pm0.7$ &$4.3\pm0.3$ &$2.6\pm0.2$ &$1.1\pm0.06\times 10^{20}$\\
&$-17.5\pm0.6$ &$1.0\pm0.07$ &$16\pm1.4$  &$9.4\pm0.8$ &$3.0\pm0.2\times 10^{19}$\\
%\hline
CO(1--0) &$2.8\pm0.2$&$7.0\times10^{-2}$&$3.5\pm0.3$&$2.1\pm 0.2$& $6.9\times 10^{13} ~ (J = 1)$\\
CO(2--1) &$2.75\pm0.17$&$3.6\times 10^{-2}$&$3.0\pm0.3$&$1.8\pm0.2$&$1.8\times10^{13} ~ (J =  2)$\\
%\hline
 & &$I~({\rm erg~ s}^{-1}~{\rm cm}^{-2}~{\rm sr}^{-1})$ & & &N({\rm {C~{\sc ii}}*})\\
%\hline
${\rm C^{+}~ 158~\mu m}$&--&$2.8\times10^{-6}$&--&--&$1.2\times10^{15}$\\
\hline
\end{tabular} 
\end{table}