\begin{table}%t1
\caption{\label{Tab:obs}Properties of IC~10.}
%\centerline
{\small
\begin{tabular}{lll}
\hline
\hline
\noalign{\smallskip}
Hubble type          &  Irr~IV                                 & 1\\
Distance             & 740 kpc                                 & 2\\
Dynamical mass       & $\sim$$1.7\times10^{9}~M_{\odot}$         & 3 \\
Stellar mass         & $\sim$$(4{-}6)\times10^{8}~M_{\odot}$         & 4, 5, 6 \\
\hi\ mass            & $\sim$$(1.7{-}2.3)\times10^{8}~M_{\odot}$     & 6, 7, 8, 9, 10 \\
H$_2$ mass           & $1\times10^7~M_{\odot}$                 & 1\\
gas fraction         & $\sim$$0.22{-}0.36$                         &  \\
$\log$(O/H) + 12     & $8.2{-}8.3$                               &11, 12, 13, 14, 15\\
$[$Fe/H$]_{\rm RGB}$ & $-1.1$                                  &16             \\
{SFR}$_{\rm H\alpha }$ & $0.2~M_{\odot }$ yr$^{-1}$              &7, 17\\
{SFR}$_{\rm FIR}$      & $0.05~M_{\odot }$ yr$^{-1}$             &18, 19\\
{SFR}$_{1.4~\rm GHz}$      &$0.07~M_{\odot }$ yr$^{-1}$              &19, 20\\
{SFR}$_{\rm PNe}$      & $0.02{-}0.04~M_{\odot }$ yr$^{-1}$        &14\\
\hline
\end{tabular}}
\tablebib{(1) van den Bergh (\cite{vdb00}); (2) Demers et~al.
(\cite{demers04}); (3) Mateo (\cite{mateo98}); (4) Jarrett et~al.
(\cite{jarrett03}); (5) Sakai et~al. (\cite{sakai99}); (6) Vaduvescu
et~al. (\cite{vaduvescu07}); (7) Gil de Paz et~al. (\cite{gil03});
(8) Huchtmeier et~al. (\cite{huchtmeier79}); (9) Wilson et~al.
(\cite{wilson96}); (10) Garnett (\cite{garnett02}); (11) Lequeux et~al. (\cite{lequeux79}); (12) Garnett (\cite{garnett90}); (13) Richer
et~al. (\cite{richer01}); (14) MG09; (15) Lozinskaya et~al.
(\cite{loz09}); (16) Kim et~al. (\cite{kim09}); (17) Kennicutt et~al. (\cite{kennicutt94}); (18) Melisse \& Israel (\cite{melisse94});
(19) Bell (\cite{bell03}); (20) White \& Becker (\cite{white92}).}\vspace*{-1.5mm}
\end{table}