\begin{table}%t1
\caption{Specific angular momentum for the last stable orbit ($j_{\rm LSO}$) around a~black hole 
with a~given mass ($M_{\rm BH}$), calculated according to Bardeen et~al. (\cite{Bardeen72}).  
Here, $j_{\rm SCH}$ and $j_{\rm Kerr,max}$ 
denote the cases for Schwarzschild black hole (non-rotating) and maximally
rotating Kerr black hole, respectively.}\label{tab:jlso}
%\centering
\small
\begin{tabular}{rcc}
\hline
\hline
     $M_{\rm BH}$ & $j_{\rm SCH}$                 & $j_{\rm Kerr,max}$ \\
                     & [${\rm cm^2~s^{-1}}$] & [${\rm cm^2~s^{-1}}$] \\
\hline
 & & \\[-8pt]
 $2.0~{M_\odot}$   & $3.07\times10^{16}$ & $1.03\times10^{16}$  \\
 $3.0~{M_\odot}$  & $4.60\times10^{16}$  & $1.55\times10^{16}$  \\
 $4.0~{M_\odot}$  & $6.13\times10^{16}$  & $2.06\times10^{16}$  \\
 $5.0~{M_\odot}$  & $7.66\times10^{16}$  & $2.57\times10^{16}$  \\
 $10.0~{M_\odot}$ & $1.53\times10^{17}$  & $5.14\times10^{16}$  \\
\hline
\end{tabular}
\end{table}