\begin{table}%t3
\caption{Stellar types expected to be observable in the central parsec, considering
the distance and the extinction towards the GC. Values taken from {\em
    Allen's Astrophysical Quantities}, the types shown here are the ones
    presented in that work that fall into the observational limits for the central parsec.}
\label{TabExpectedStars}
%\centering
\par
\begin{tabular}{l r r l r r}
\hline\hline
Early types & mag $K$ & $T_{\rm eff}$ & Late types & $T_{\rm eff}$ & mag $K$ \\
\hline
B3Ia & 11.80 & $\sim$16~000 & M6III & $\sim$3200 & 10.78 \\
O6I & 12.12 & $\sim$36~000 & M4III & $\sim$3400 & 12.32 \\
O7V & 13.92 & $\sim$36~000 & M2III & 3540 & 12.92 \\
B0V & 14.65 & 30~000 & M0III & 3690 & 13.57 \\
B2V & 16.03 & 20~900 & K4.5III & $\sim$4100 & 14.29 \\
B3V & 16.33 & $\sim$19~000 & K2.5III & $\sim$4300 & 15.37 \\
B7V & 17.51 & $\sim$13~000 & G8.5III & $\sim$4750 & 16.42 \\
 & & & G7III & $\sim$4900 & 16.50 \\
 & & & G5III & 5050 & 16.62 \\
 & & & G4III & $\sim$5100& 16.77 \\
 & & & G0III & $\sim$5200& 17.27 \\
\hline
\end{tabular}
\end{table}