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\begin{table*}
\caption[ ]{ ASCA upper limits of X--ray emission from K~416 members}
\begin{flushleft}
\begin{tabular}{l c c c c c l }
\noalign{\smallskip}
\hline
\noalign{\smallskip}
Object  & counts~s$^{-1}$ & Flux$_{(0.3 - 1 0 {\rm keV})}$        & L$_{(0.3
- 10 {\rm keV})}$
	& Flux$_{(0.3 - 2.4 {\rm keV})}$  & L$_{(0.3 - 2.4 {\rm keV})}$      &
	detector   \cr
	&(10$^{-3}$)      & (10$^{-13}$ergs~s$^{-1}$~cm$^{-2}$) &
	(10$^{41}$ h$^{-1}_{50}$ ergs~s$^{-1}$)
	& (10$^{-13}$ergs~s$^{-1}$~cm$^{-2}$) &
	(10$^{41}$ h$^{-1}_{50}$ ergs~s$^{-1}$) &            \cr
\noalign{\smallskip}
\hline
\noalign{\smallskip}
NGC~5480  &  $<1.4 $ & $<1.0$ &  $<0.2$ &  $<0.5$  & $<0.1$  & GIS~2
\cr
NGC~5480  &  $<3.0 $ & $<1.7$ &  $<0.3$ &  $<0.9$  & $<0.2$   &
GIS~3    \cr
	  &       &        &         &          &          &
	  \cr
NGC~5481  & $<1.4 $  & $<0.9$ &  $<0.2$ & $<0.8$   & $<0.2$   &
GIS~2    \cr
NGC~5481  & $<2.6 $  & $<1.4$ &  $<0.3$ & $<1.2$   & $<0.3$   &
GIS~3    \cr
	  &       &        &         &          &          &
	  \cr
Extended  & $<3.3$   & $<2.0$ &  $<0.4$ & $<1.9$   & $<0.4$   & GIS~2
\cr
Emission  & $<5.0 $  & $<2.6$ &  $<0.5$ & $<2.4$   & $<0.5$   & GIS~3
\cr
\noalign{\smallskip}
\hline
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\end{tabular}
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{{\bf Notes}: 3 $\sigma$ upper limits have been calculated in a circle
of 2\farcm5 for the two galaxies and of 7\farcm5 for the extended
emission, as explained in the text.  Fluxes are derived
assuming a thermal bremsstrahlung model
with $kT$=5~keV for NGC~5480 and a Raymond Smith plasma model
with $kT$=1~keV and abundance = 0.5 solar for NGC~5481 and the extended
source.$N_H$ has been taken from Stark et al.  (1992) = 1.41 $\times$
10$^{20}$ cm$^{-2}$.  A distance of 40 $h^{-1}_{50}$ Mpc is assumed.}
\end{table*}
%--------------------------end Table1-----------------------------------------


%--------------------------Table2--------------------------------------------
\begin{table}
\begin{flushleft}
\caption[]{Main kinematics data}
\begin{tabular}{l l l l l}
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\hline
\noalign{\smallskip}
ident.      &  other ident. & V$_{{\rm hel}}$    & $\sigma_0$ & Type \cr
	    &               & km~s$^{-1}$  & km~s$^{-1}$&       \cr
\noalign{\smallskip}
\hline
\noalign{\smallskip}
NGC~2300    &               &   2003$\pm$34&  330(1)  &  E2
\cr
	    &                   &                            &
	    &       \cr
HCG~62a     &                   &   4279$\pm$25   &
246$\pm$24          &   E3    \cr
HCG~62b      &                  &   3542$\pm$25   &
272$\pm$26         &  S0     \cr
	    &                   &                            &
	    &       \cr
HCG~68a      &   NGC~5353 &   2250$\pm$22&   361$\pm$22         &
S0    \cr
HCG~68b      &  NGC~5354  &   2570$\pm$17&    241$\pm$22        &
E2    \cr
	    &             &                      &              &
	    \cr
K~416b        &  NGC~5481   &   2033$\pm$13   &   185$\pm$14       &
E3     \cr
\noalign{\medskip \hrule}
\end{tabular}
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\medskip
{\bf Notes:} (1) The central velocity dispersion of NGC~2300 is extrapolated.
\end{table}
%--------------------------end Table2------------------------------------------

%--------------------------Table3--------------------------------------------
\begin{table*}
\caption[ ]{ Positions and parameters of the fit of X--ray spectra of
unknown sources}
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\begin{tabular}{c c c c  c c c c c c}
\noalign{\smallskip}
\hline
\noalign{\smallskip}
Object  & R.A.       & $\delta$   & Counts/s      &  $\gamma$  &  norm. 
& $\chi^2$ & bins & Flux$_{(0.3 - 1 0 {\rm keV})}$ & Camera\cr
	    & (2000)  & (2000)       &  (10$^{-3}$) &
	    &   (10$^{-5}$)        &                 
&        &	    (10$^{-13} $ erg~cm$^{-2}$~{\rm s}$^{-1}$) &            \cr
\noalign{\smallskip}
\hline
\noalign{\smallskip}
Unknown source 1  &   14~05~12  &  50~42~29 & &                                 
&        &       &       &        & GIS~2 \cr
                             &    14~05~04 &  50~41~36  &  4.4$\pm$0.5  & 
2.3$^{+2.0}_{-0.8}$ & 9.4  & 0.8 & 15  &
			      4.7  & GIS~3   \cr
			      &
			      &                    &
			      &
			      &        &       &       &
			      &            \cr
Unknown source 2  &   14~05~37 &  50~56~51 &
&                                  &        &       &       &        &
GIS~2  \cr
			      &    14~05~29 & 50~56~11 &
			      4.0$\pm$0.4& 1.8 $^{+0.9}_{-0.3}$ &
			      6.8 & 0.8 & 16 & 3.7 & GIS~3  \cr
\noalign{\smallskip}
\hline
\noalign{\smallskip}
\end{tabular}
\end{flushleft}
{\bf Notes}:  GIS~3 spectra were tentatively fitted with a power law, $\gamma$,
and interstellar absorption,   N$_H$ = 0 and 1.1~10$^{21}$ cm$^{-2}$
respectively for the source 1 and 2. The errors  are computed on two degrees of
freedom 90\% confidence interval. 
\end{table*}
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