\begin{table}%t2
\caption{Results for Henize 2-10.}\label{tab:obs1}
\par
%\begin{center}
\par
\begin{tabular}{c|cccccc}
\hline\hline
\textbf{Henize~2-10}&&&&&&\\
\hline
Transition & Freq. & Beam size & $\int(T_{\rm mb}{\rm d}v)$ & Intensity & Flux & References$^{a}$\\
      &(GHz) & ($\arcsec$) & (K~km~s$^{-1}$) & (W~m$^{-2}$~sr$^{-1}$) & (W~m$^{-2}$) &\\
\hline
CI($^{3}$P$_{1}$--$^{3}$P$_{0}$) & 492.162 &14.55 & $4.2\pm 0.8$ & $5.1\times10^{-10}$ & $3.0\times10^{-18}$ & 4 and 5$^{b}$\\
      & & 21.90 & $2.5\pm0.5$ & $3.0\times10^{-10}$ & $3.8\times10^{-18}$ & 4 and 5$^{b}$\\ 
\hline
$^{12}$CO(1--0) & 115.271 & 40.00 & $10.0\pm0.8$ & $1.6\times10^{-11}$ & $6.7\times10^{-19}$ & 1\\
& & 21.90 & $27.3\pm2.2$ & $4.3\times10^{-11}$ & $5.5\times10^{-19}$ & 1\\ 
      &  & 55.00 & $4.9\pm0.2$ & $7.6\times10^{-12}$& $6.1\times10^{-19}$ & 2\\
      & & 21.90 & $23.9\pm1.0$& $3.7\times10^{-11}$ &$4.8\times10^{-19}$ & 2*\\
      $^{12}$CO(2--1) & 230.538 & 21.00 & $17.3\pm1.4$ & $2.2\times10^{-10}$ & $2.5\times10^{-18}$ & 1*\\
      &  & 27.00 & $6.8\pm0.8$ & $8.5\times10^{-11}$ & $1.7\times10^{-18}$ & 2\\
      & & 21.90 & $9.4\pm1.1$ & $1.2\times10^{-10}$ & $1.5\times10^{-18}$ & 2\\
      $^{12}$CO(3--2) & 345.796 & 21.90 & $11.5\pm2.3$ & $4.9\times10^{-10}$ & $6.2\times10^{-18}$ &5* \\
      & & 21.00 & $23.2\pm2.1$ & $9.8\times10^{-10}$ & $1.2\times10^{-17}$ & 1\\
      &  & 22.00 & $16.6\pm0.6$ & $7.0\times10^{-10}$ & $9.0\times10^{-18}$ & 3\\
      $^{12}$CO(4--3) & 461.041 & 14.55 & $18.6\pm4.2$ & $1.9\times10^{-9}$ & $1.1\times10^{-17}$ &5 \\
      & & 21.90 & $10.9\pm2.4$ & $1.1\times10^{-9}$ & $1.4\times10^{-17}$ & 5*\\
      $^{12}$CO(6--5) & 691.473 & 10.60 & $15.7\pm3.1$ & $5.3\times10^{-9}$ & $1.6\times10^{-17}$ & 5\\
      & & 21.90 & $6.8\pm1.3$ & $2.3\times10^{-9}$ & $2.9\times10^{-17}$ & 5*\\
      $^{12}$CO(7--6) & 806.652 & 8.95 & $15.2\pm3.0$ & $8.2\times10^{-9}$ & $1.7\times10^{-17}$ & 5\\
      &  & 21.90 & $5.8\pm1.2$ & $3.1\times10^{-9}$ & $4.0\times10^{-17}$ & 5*\\
\hline
      $^{13}$CO(1--0) & 110.201 & 40.00 & $<$0.5 & $<$$6.8\times10^{-13}$& $<$$2.9\times10^{-20}$ & 1 \\
      &  & 21.90 & $<$1.4 & $<$$1.8\times10^{-12}$ & $<$$2.4\times10^{-20}$ & 1\\
      &  & 57.00 & $0.3\pm0.1$ & $3.9\times10^{-13}$ & $3.4\times10^{-20}$ & 2\\
      &  & 21.90 & $1.6\pm0.5$ & $2.2\times10^{-12}$ & $2.8\times10^{-20}$ & 2*\\
      $^{13}$CO(2--1) & 220.399 & 21.00 & $0.9\pm0.2$ & $9.9\times10^{-12}$ & $1.2\times10^{-19}$ & 1*\\
      $^{13}$CO(3--2) & 330.588 & 14.00 & $2.3\pm0.6$& $8.5\times10^{-11}$ & $4.4\times10^{-19}$ & 1\\
      &  & 21.90 & $1.3\pm0.3$ & $4.8\times10^{-11}$ & $6.1\times10^{-19}$ & 1*\\
      &  & 21.90 & $1.8\pm0.5$ & $6.7\times10^{-11}$ & $8.5\times10^{-19}$ & 5\\
\hline
\end{tabular}
%\end{center}
\par
$^{a}$~References: 1:~Baas et~al.~(\cite{Baas94}); 2:~Kobulnicky et~al.~(\cite{Kobulnicky95}); 3:~Meier et~al.~(\cite{Meier01}); 4:~Gerin \& Phillips~(\cite{Gerin00}); 5:~this work; *:~used for models.\\
$^{b}$~We analysed again spectra from Gerin \& Phillips~(\cite{Gerin00}).
\end{table}