\begin{table}%t6
\caption{\label{nh3gauss}\nh\ line parameters obtained from the Gaussian fits to the \nh~(1, 1) and (2, 2).}
%\centering
\small
\begin{tabular}{lcccccccccc}
\hline\hline
&\multicolumn{2}{c}{Position}
&
&\multicolumn{3}{c}{Main line}
&
&\multicolumn{2}{c}{Inner satellites}
&\\
\cline{2-3}
\cline{5-7}
\cline{9-10}
&$\alpha$ (J2000) &$\delta$ (J2000)
&Transition
&\vel
&$\Tmb$
&$\Delta~v$
&
&$\Tmb$
&$\Delta~v$
&$\frac{\Tmb~(m)}{\Tmb~(is)}$
\\
Source
&(h m s)
&($\degr$ $'$ $''$)
&$(J,K)$
&(\kms)
&(K)
&(\kms)
&
&(K)
&(\kms)
&
\\
\hline
VLA~8A &00 24 11.01 &$+$65 47 09.9  &$(1,1)$ &$-19.98\pm0.01$ &3.9~$\pm$~0.2  &$1.19\pm0.02$ &&1.8~$\pm$~0.2 &1.14~$\pm$~0.04  &2.2 \\
	&&			     &$(2,2)$ &$-19.92\pm0.03$ &1.8~$\pm$~0.1  &$0.83\pm0.07$ &&  &  & \\ 
\hline	
VLA~8B	&00 24 11.76  &$+$65 47 09.8 &$(1,1)$ &$-19.89\pm0.01$ &3.6~$\pm$~0.2  &$1.16\pm0.02$ &&1.5~$\pm$~0.2 &1.18~$\pm$~0.06 &2.4  \\ 
	&&			     &$(2,2)$ &$-19.88\pm0.04$ &1.5~$\pm$~0.1  &$0.91\pm0.08$ &&  &  & \\
\hline
IRS~1	&00 24 10.10  &$+$65 47 09.1 &$(1,1)$ &$-19.97\pm0.02$  &2.2~$\pm$~0.1  &$1.19\pm0.03$ &&1.0~$\pm$~0.1 &1.11~$\pm$~0.07 &2.2\\
	&&			     &$(2,2)$ &$-19.83\pm0.05$  &1.0~$\pm$~0.1  &$0.92\pm0.08$ &&  &  & \\ 
\hline
MM2	&00 24 12.30  &$+$65 46 45.0 &$(1,1)$ &$-19.84\pm0.02$ &1.4~$\pm$~0.1  &$1.19\pm0.05$ &&0.9~$\pm$~0.1 &1.06~$\pm$~0.05 &1.6 \\ 
	&&  		       	     &$(2,2)$ &$-19.85\pm0.08$ &0.5~$\pm$~0.1  &$0.88\pm0.17$ &&  &  & \\   
\hline
MM1	&00 24 10.80  &$+$65 47 06.0 &$(1,1)$ &$-19.94\pm0.01$ &4.8~$\pm$~0.2   &$1.10\pm0.03$ &&2.5~$\pm$~0.1   &1.02~$\pm$~0.04   &1.9 \\ 
	&& 			     &$(2,2)$ &$-19.96\pm0.04$ &1.8~$\pm$~0.1   &$0.83\pm0.10$ &&  &  & \\  
\hline
SC	&00 24 05.30  &$+$65 47 47.0  &$(1,1)$ &$-19.95\pm0.01$ &2.7~$\pm$~0.1  &$0.97\pm0.02$   &&1.5~$\pm$~0.1 &0.95~$\pm$~0.05 &1.8 \\
\par
\hline
\end{tabular}
\end{table}