\begin{table}%t3
\caption{Comparison of the specific angular momentum of the accreted material to the
Keplerian specific angular momentum at the magnetospheric radius. An estimation of the flux for the onset of centrifugal inhibition of accretion is also shown.}\label{angular} 
%\centerline
{\begin{tabular}{p{1.3cm} l l} 
\hline \hline\noalign{\smallskip}
& $B= 16.5\times10^{12}$~G &  $B= 1.65 \times 10^{12}$~G\\
&(4.5--6.5)~kpc &(4.5--6.5)~kpc\\
\hline \noalign{\smallskip}
$k=0.91$  &  $\ell = (0.61$--0.33) $\ell_{m}$&$\ell= (1.19$--0.63) $\ell_{m}$ \\
&  $F_{\min}^*=  (20.4$--9.8) & $F_{\min}^*=   (0.2$--0.097)\\
$k=0.47$  & $\ell= (0.85$--0.45) $\ell_m$ & $\ell= (1.65$--0.88) $\ell_{m}$ \\
&$F_{\min}^*= (2.02$--0.97) & $F_{\min}^*=   (0.02$--0.0097)\\
\hline 
\end{tabular} }
\smallskip
 $^* \times 10^{-12}$~{\rm erg~cm}$^{-2}$~{\rm s}$^{-1}$. 
\end{table}