\begin{table}%T1
\caption{\label{tab:prop}Observational properties of Pox~36.}
\small%\centering
\par
\begin{tabular}{l l l }
\hline\hline
Property     &  Value         &   Comment          \\ 
\hline  
$\alpha$ (J2000) & $11{\rm h}58{\rm m}57.3{\rm s}$ &           HIPASS (Meyer et~al.\ \cite{Meyer2004}) \\
$\delta$ (J2000) & $-19^\circ01'41''$ &           HIPASS (Meyer et~al.\ \cite{Meyer2004}) \\
Galactic coordinates & $l=286.114$, $b=42.123$ &              HIPASS (Meyer et~al.\ \cite{Meyer2004}) \\
\hline
Foreground Galactic extinction (mag) & $E(B-V)=0.038$  & Schlegel et~al.\ (\cite{Schlegel1998})  \\ 
\hline
Magnitude (mag) & $B_J=14.27$, $I=14.38$  & HIPASS (Doyle et~al.\ \cite{Doyle2005}) \\
                    & $K_{\rm s}=12.63$                     & Vanzi \& Sauvage (\cite{Vanzi2006}) \\
\hline\noalign{\smallskip}
$L$(H$\beta$) (erg s$^{-1}$) &  $1.81\times10^{39}$   & From $F$(H$\beta$) (Izotov \& Thuan \cite{Izotov2004}) and $D = 20$~Mpc \\
\hline
{\it FWHM} (H{~\sc i})  (\kms) & $67.4$ &                     HIPASS (Meyer et~al.\ \cite{Meyer2004}) \\
Peak H{~\sc i}~flux (Jy) & $0.1197$ &                     HIPASS (Meyer et~al.\ \cite{Meyer2004}) \\
Integrated H{~\sc i}~flux (Jy\kms) & $8.6$ &                      HIPASS (Meyer et~al.\ \cite{Meyer2004}) \\
$M$(H{~\sc i}) ($M_\odot$)     & $8.1\times10^8$                &   Derived from the H{~\sc i}~flux with the distance = $20$~Mpc \\
\hline
Radial velocity (\kms)   &    $1114\pm2$  &   21~cm line, Theureau et~al.\ (\cite{Theureau1998}) \\ 
                               & $1113.9\pm6.5$ &                      HIPASS (Meyer et~al.\ \cite{Meyer2004}; Zwaan et~al.\ \cite{Zwaan2004}) \\
& $1065\pm20$ & Optical lines (Izotov \& Thuan \cite{Izotov2004}) \\
\hline
Distance (Mpc)   & $\approx$$12$           &    Vigroux et~al.\ (\cite{Vigroux1987}) with $H_0=73$\kms  \\
	         & $\approx$$16$      &    Kunth \& Joubert (\cite{Kunth1985})\\
	         & $\approx$$20$      &    Using $v=1114$\kms, $H_0=73$\kms, $\Omega_{\rm m}=0.27$   \\
\hline
$\log$ O/H  & $-3.95\pm0.02$&                  Izotov \& Thuan (\cite{Izotov2004}) \\ 
     & $-3.86\pm0.03$ &                    Kobulnicky \& Skillman (\cite{Kobulnicky1996}) \\
     & $-3.81\pm0.04$ &                    Campbell (\cite{Campbell1988}, \cite{Campbell1992}) \\
     & $-3.82\pm0.04$ &                    Kunth \& Sargent (\cite{Kunth1983}) \\
$\log$ N/H  & $-5.53\pm0.03$ &                    Izotov \& Thuan (\cite{Izotov2004}) \\ 
     & $-5.39\pm0.10$ &                     Kobulnicky \&  Skillman (\cite{Kobulnicky1996}) \\
     & $-5.38\pm0.05$ &                      Campbell (\cite{Campbell1992})   \\
     & $-5.37\pm0.05$ &                    Kunth \& Sargent (\cite{Kunth1983}) \\
$\log$ Ar/H & $-6.24\pm0.03$ &                     Izotov \& Thuan (\cite{Izotov2004}) \\ 
$\log$ Fe/H & $-6.17\pm0.10$ &                     Izotov \& Thuan (\cite{Izotov2004}) \\ 
\hline
\end{tabular}
\end{table}