\begin{table}%t2
\caption{Angular diameter, stellar radius and rotational period.\label{tab2}}
$$
\begin{array}{lclclclclcl}
\hline
\hline
{\rm HD} & & \Theta^{a} & & \Theta^{b} & & d   && R/R_{\sun}~^{c} & & P_{{\rm rot}}/\sin{i}   \\ 
{\rm }   & & {\rm mas}      & &  {\rm mas}     & & {\rm pc} & & & & {\rm day}    \\ 
\hline
21~120  & & 2.64 & & 2.26 & &  64.85  & & 18.4 & & 143 \\
22~663  & & 2.06 & & 1.76 & &  67.20  & & 14.9 & & 533 \\
23~319  & & 2.73 & & 2.18 & &  54.53  & & 16.0 & & 569 \\
27~371  & & 2.69 & & 2.56 & &  47.24  & & 13.6 & & 253 \\
27~697  & & 2.57 & & 2.43 & &  46.97  & & 12.9 & & 190 \\
32~887  & & 6.20 & & 6.29 & &  69.49  & & 46.3 & & {>}2357  \\
47~536  & & 1.81 & & 1.59 & &  121.36 & & 23.6 & & 625 \\
50~778  & & 4.22 & & 3.88 & &  77.28  & & 35.5 & & {>}1807  \\
61~935  & & 2.55 & & 2.35 & &  44.33  & & 12.1 & & 326 \\
62~902  & & 1.84 & & 1.90 & &  73.10  & & 14.4 & & {>}733  \\
63~697  & & 1.99 & & 1.89 & &  77.70  & & 16.6 & & {>}845  \\
65~695  & & 2.07 & & 1.92 & &  76.57  & & 17.1 & & {>}870  \\
81~797  & & 10.66& & 10.52 & &  54.35  & & 62.3 & & 2991 \\
90~957  & & 1.87 & & 1.95 & &  118.76 & & 23.9 & & {>}1217  \\
99~167  & & 3.72 & & 3.77 & &  111.73 & & 44.7 & & {>}2775  \\
110~014 & & 2.21 & & 2.26 & &  97.66  & & 23.2 & & 1036 \\
113~226 & & 3.78 & & 3.47 & &  31.35  & & 12.7 & & 173 \\ 
115~478 & & 1.93 & & 1.81 & &  91.41  & & 18.9 & & {>}962  \\
124~882 & & 3.87 & & 2.89 & &  85.47  & & 35.6 & & {>}1812  \\
125~560 & & 2.07 & & 2.05 & &  58.41  & & 13.0 & & 848 \\
151~249 & & 7.94 & & 6.09 & &  96.06  & & 82.0 & & {>}4174  \\
189~319 & & 6.67 & & 7.09 & &  84.03  & & 60.2 & & {>}3064  \\
\hline
\end{array} 
$$
\smallskip
$^{a}$ CHARM catalogue (Richichi \& Percheron \cite{ric02}). \\
$^{b}$ This work. \\
$^{c}$ Computed using $\Theta^{(a)}$. \\
For stars with undetermined $v_{{\rm rot}} \sin{i}$ we computed 
the lower limit for $P_{{\rm rot}}/\sin{i}$ by assuming 
$v_{{\rm rot}} \sin{i} = \; 1\; {\rm km~s}^{-1}$.
\end{table}