\begin{table}%ta3
    %\centering
\par
    \caption{\label{t:mirasobsresults}Observational results of circumstellar CO and SiO~line emission 
              towards our Mira sample.}
        %\centering
\par
        {
	\begin{tabular}{llcrcccc}
\hline\hline
\noalign{\smallskip}
GCVS4 & IRAS  & Molecule &Code & $I$ & $T_{\rm mb}$ & $v_{\rm LSR}$ &  $v_{\rm e}$ \\
      &       &    &     & [K~km~s$^{-1}$] & [K]  & [km~s$^{-1}$] & [km~s$^{-1}$] \\
\noalign{\smallskip}\hline\noalign{\smallskip}
TX Cam   & 04566+5606 &CO &O10& {\phantom{1}}21.5 & 0.88 & 11.5 & 20.0 \\
         &            &   &I10& {\phantom{1}}67.0 & 1.44 & 11.5 & 21.0 \\
         &            &   &I21&             241.3 & 3.93 & 11.4 & 20.7 \\
         &            &   &J21& {\phantom{1}}69.7 & 2.61 & 11.4 & 20.2 \\
         &            &   &J32&             167.2 & 6.14 & 11.3 & 20.3 \\
         &            &SiO&O21& {\phantom{1}}13.2 & 0.52 & 10.7 & 18.6 \\
\par
R Cas    & 23558+5106 &CO &O10& {\phantom{11}}8.4 & 0.46 & 24.9 & 12.2 \\
         &            &   &J21& {\phantom{1}}32.1 & 1.78 & 24.8 & 11.1 \\
         &            &   &J32& 	    100.2 & 5.48 & 25.2 & 11.0 \\
         &            &   &J43& {\phantom{1}}89.6 & 5.44 & 24.8 & 11.9 \\
         &            &SiO&O21& {\phantom{11}}8.6 & 0.67 & 26.3 & 9.4 \\
\par
R Hya    & 13269--2301&CO &S10& {\phantom{11}}0.6 & 0.09: & $-$9.7: & 5.3: \\
	     &            &   &J32& {\phantom{1}}43.0 & 3.65 & $-$10.5 & 8.6 \\
	     & 	          &SiO&S21& {\phantom{11}}2.8 & 0.44 & $-$11.5 & 5.2 \\
	     & 	          &   &S54& {\phantom{11}}7.7 & 1.30 & $-$11.2 & 5.9 \\	     
\par
R Leo    & 09448+1139 &CO &O10& {\phantom{11}}2.4 & 0.25 & 0.2 & 7.4\\
         &            &   &J21& {\phantom{1}}15.0 & 1.30 & $-$0.4 & 8.7 \\
         &            &   &J32& {\phantom{1}}41.6 & 3.88 & $-$0.3 & 7.8 \\
         &            &SiO&O21& {\phantom{11}}5.1 & 0.51 & 0.5 & 6.8 \\
         &            &   &S21& {\phantom{11}}4.9 & 0.65 & 0.2 & 6.9 \\
	     & 	          &   &S54& {\phantom{1}}10.8 & 1.58 & 0.4 & 6.3 \\         
\par
GX Mon   & 06500+0829 &CO &O10& {\phantom{1}}49.6 & 1.55 & $-$9.3 & 24.4 \\
	     &	          &   &J21& {\phantom{1}}67.2 & 2.27 & $-$9.5 & 18.2 \\
         &            &   &J32& {\phantom{1}}87.6 & 2.96 & $-$9.4 & 17.9 \\
         &            &   &J43& {\phantom{1}}56.2 & 1.82 & $-$8.7 & 17.5 \\
         &            &SiO&O21& {\phantom{11}}9.4 & 0.36 & $-$9.6 & 19.5 \\
         &            &   &S21& {\phantom{11}}5.5 & 0.29 & $-$9.6 & 18.9 \\
         &            &   &S54& {\phantom{11}}8.9 & 0.42 & $-$9.1 & 18.7 \\                  
\par
WX Psc   & 01037+1219 &CO &O10& {\phantom{1}}52.0 & 1.61 & 9.6 & 18.6 \\
	     &	          &   &J21& {\phantom{1}}31.0 & 1.31 & 10.1 & 18.3 \\
         &            &   &J32& {\phantom{1}}45.5 & 1.63 & 9.5 & 20.8 \\
         &            &   &J43& {\phantom{1}}49.9 & 1.82 & 9.5 & 20.6 \\
	     &            &SiO&O21& {\phantom{1}}10.0 & 0.40 & 10.1 & 18.9 \\
         &            &   &S21& {\phantom{11}}5.6 & 0.22 & 9.3 & 19.2 \\ 
         &            &   &S54& {\phantom{11}}6.8 & 0.29 & 9.3 & 17.7 \\          	     
IK Tau   & 03507+1115 &CO &O10& {\phantom{1}}58.6 & 1.70 & 34.4 & 17.2 \\
	     &	          &   &J21& 	    103.8 & 3.32 & 34.5 & 17.5 \\
         &            &   &J32& 	    143.8 & 4.81 & 34.2 & 17.6 \\
         &            &   &J43& 	    127.0 & 4.52 & 33.2 & 18.0 \\
	     & 	          &SiO&O21& {\phantom{1}}16.1 & 0.66 & 33.9 & 18.1 \\
         &            &   &S54& {\phantom{1}}18.9 & 0.73 & 34.7 & 17.5 \\
         &            &   &S65& {\phantom{1}}13.7 & 0.61 & 34.7 & 15.9 \\
\par
IRC+10365& 18349+1023 &CO &O10& {\phantom{1}}21.5 & 0.79 & $-$31.3 & 16.9 \\
         &            &   &J21& {\phantom{1}}42.0 & 1.48 & $-$30.7 & 15.3 \\
         &            &SiO&O21& {\phantom{11}}6.3 & 0.30 & $-$32.6 & 15.6 \\
\par
IRC--10529& 20077--0625&CO &O10& {\phantom{1}}15.7 & 0.65 & $-$18.1 & 15.7 \\
         &            &   &J21& {\phantom{1}}24.4 & 1.18 & $-$17.5 & 17.7 \\
         &            &   &J32& {\phantom{1}}48.0 & 2.22 & $-$17.1 & 14.2 \\
         &            &   &J43& {\phantom{1}}57.4 & 2.87 & $-$17.2 & 16.0 \\
	 &	      &SiO&O21& {\phantom{11}}2.9 & 0.16 & $-$17.7 & 14.6 \\
\par
IRC--30398& 18560--2954&CO &J21& {\phantom{1}}44.6& 1.76 & $-$6.4 & 19.4 \\
	 &	       &SiO&S21& {\phantom{11}}0.8& 0.06: & $-$10.1: & 15.3:\\
\par
IRC+40004& 00042+4248 &CO &O10& {\phantom{1}}24.8 & 0.82 & $-$20.5 & 19.2 \\
         &            &   &J21& {\phantom{1}}41.5 & 1.41 & $-$20.5 & 18.9 \\
  	 &	      &SiO&O21& {\phantom{11}}1.3 & 0.05 & $-$21.3 & 20.3 \\
\par
IRC+50137& 05073+5248 &CO &J21& {\phantom{1}}36.8 & 1.40 & 3.5 & 18.7 \\
         &            &   &J32& {\phantom{1}}35.7 & 1.32 & 3.3 & 18.1 \\
         &	      &SiO&O21& {\phantom{11}}2.0 & 0.10 & 1.4 & 14.4 \\
\hline
\end{tabular}}
\end{table}