\begin{table*}
%\centering
\par
\caption{For those stars for which we have a parallax obtained by
Hipparcos, we derive the distance $D$ (pc) and the luminosity $L$
($10^3~L_{\odot}$) based on that parallax. In the second part of the
table, distance and luminosity estimates are given based on the P-L
relation of \citet{98Alcock}. Periods $P$ (days) are from SIMBAD and
bolometric corrections ${\it BC}_V$ from \citet{98Bessell}. The luminosity
$L$ (in $10^3~L_{\odot}$) and the distance $D$ (in kpc) are given
together with the estimated errors. Where we don't have a pulsation
period, distances are estimated based on a luminosity of $L =
5000\pm2000~L_{\odot}$.\label{tab:distances}}
$$
\begin{tabular}{ll|r@{~$\pm$~}lcc|crr@{~$\pm$~}lr@{~$\pm$~}l}
\hline
\hline
No	&Name			&\multicolumn{2}{c}{Parallax}	&Distance $D$		&$L$
&Period $P$	&${\it BC}_V$		&\multicolumn{2}{c}{$L$}			&\multicolumn{2}{c}{Distance $D$}\\
	&			&\multicolumn{2}{c}{(mas)}	&(pc)			&($10^3~L_{\odot}$)
&(days)		&		&\multicolumn{2}{c}{($10^3~L_{\odot}$)}	&\multicolumn{2}{c}{(kpc)}\\
\hline
1	&TW~Cam		&\multicolumn{2}{c}{}		&			&
&$85.6$		&$-0.36$	&$3.8$		&$2.6$				&$2.8$		&$1.0$\\
\par
2	&RV~Tau		&\multicolumn{2}{c}{}		&			&
&$78.698$	&$-0.51$	&$3.8$		&$2.6$				&$2.1$		&$0.7$\\
\par
3	&IRAS~05208		&\multicolumn{2}{c}{}		&			&
&		&$-0.98$	&\multicolumn{2}{c}{}				&$4.1$		&$0.8$\\
\par
4	&DY~Ori		&\multicolumn{2}{c}{}		&			&
&$60.26$	&$0.00$		&$1.6$		&$1.0$				&$1.9$		&$0.6$\\
\par
5	&CT~Ori		&\multicolumn{2}{c}{}		&			&
&$135.52$	&$-0.08$	&$6.0$		&$4.5$				&$6.6$		&$2.5$\\
\par
6	&SU~Gem		&\multicolumn{2}{c}{}		&			&
&$50.12$	&$-0.03$	&$1.2$		&$0.8$				&$2.2$		&$0.7$\\
\par
7	&UY~CMa		&\multicolumn{2}{c}{}		&			&
&$113.9$	&$-0.08$	&$4.5$		&$3.3$				&$8.5$		&$3.1$\\
\par
8	&HD~44179		&$2.62$		&$2.37$		&$200$--$382$--$4000$	&$0.01$--$0.03$--$3.81$
&		&$0.11$		&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{$< $4.6}\\
\par
9	&HD~46703		&\multicolumn{2}{c}{}		&			&
&		&$0.06$		&\multicolumn{2}{c}{}				&$4.3$		&$0.9$\\
\par
10	&ST~Pup		&\multicolumn{2}{c}{}		&			&
&$18.8864$	&$-0.01$	&$0.3$		&$0.1$				&$1.3$		&$0.4$\\
\par
11	&HD~52961		&\multicolumn{2}{c}{}		&			&
&		&$0.04$		&\multicolumn{2}{c}{}				&$2.3$		&$0.5$\\
\par
12	&SAO~173329		&\multicolumn{2}{c}{}		&			&
&		&$0.11$		&\multicolumn{2}{c}{}				&$7.0$		&$1.5$\\
\par
13	&U~Mon			&$1.45$		&$0.82$		&$441$--$690$--$1587$	&1.21$-$2.96$-$15.65
&$92.26$	&$-0.24$	&$3.8$		&$2.7$				&$0.8$		&$0.3$\\
\par
14	&AR~Pup		&$2.75$		&$1.16$		&$256$--$364$--$629$	&0.03$-$0.06$-$0.17
&$75$		&$0.00$		&$2.2$		&$1.5$				&\multicolumn{2}{c}{$< $1.8}\\
\par
15	&IRAS~08544		&\multicolumn{2}{c}{}		&			&
&		&$0.11$		&\multicolumn{2}{c}{}				&$0.8$		&$0.2$\\
\par
16	&IRAS~09060		&\multicolumn{2}{c}{}		&			&
&		&$0.08$		&\multicolumn{2}{c}{}				&$4.4$		&$0.9$\\
\par
17	&IRAS~09144		&\multicolumn{2}{c}{}		&			&
&		&$-0.01$	&\multicolumn{2}{c}{}				&$2.7$		&$0.6$\\
\par
18	&IW~Car		&\multicolumn{2}{c}{}		&			&
&$67.5$		&$0.08$		&$1.7$		&$1.2$				&$0.7$		&$0.2$\\
\par
19	&IRAS~09400		&\multicolumn{2}{c}{}		&			&
&		&		&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{}\\
\par
20	&IRAS~09538		&\multicolumn{2}{c}{}		&			&
&		&$-0.08$	&\multicolumn{2}{c}{}				&$7.7$		&$1.6$\\
\par
21	&HR~4049		&$1.50$		&$0.63$		&$469$--$667$--$1149$	&$1.67$--$3.39$--$10.05$
&		&$0.11$		&\multicolumn{2}{c}{}				&$0.8$		&$0.2$\\
\par
22	&IRAS~10174		&\multicolumn{2}{c}{}		&			&
&		&		&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{}\\
\par
23	&IRAS~10456		&$1.18$		&$0.60$		&$562$--$847$--$1724$	&$3.31$--$7.52$--$31.15$
&		&$-0.70$	&\multicolumn{2}{c}{}				&$0.7$		&$0.1$\\
\par
24	&HD~95767		&\multicolumn{2}{c}{}		&			&
&		&$0.10$		&\multicolumn{2}{c}{}				&$2.0$		&$0.4$\\
\par
25	&GK~Car		&\multicolumn{2}{c}{}		&			&
&$55.6$		&		&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{}\\
\par
26	&IRAS~11472		&\multicolumn{2}{c}{}		&			&
&		&$-0.03$	&\multicolumn{2}{c}{}				&$9.7$		&$2.0$\\
\par
27	&RU~Cen		&\multicolumn{2}{c}{}		&			&
&$64.727$	&$0.00$		&$1.7$		&$1.2$				&$1.6$		&$0.6$\\
\par
28	&SX~Cen		&\multicolumn{2}{c}{}		&			&
&$32.8642$	&$0.02$		&$0.6$		&$0.4$				&$1.3$		&$0.4$\\
\par
29	&HD~108015		&\multicolumn{2}{c}{}		&			&
&		&$0.11$		&\multicolumn{2}{c}{}				&$2.5$		&$0.5$\\
\par
30	&IRAS~13258		&\multicolumn{2}{c}{}		&			&
&		&		&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{}\\
\par
31	&EN~TrA		&\multicolumn{2}{c}{}		&			&
&$36.9$		&$0.02$		&$0.7$		&$0.4$				&$1.1$		&$0.3$\\
\par
32	&IRAS~15469		&\multicolumn{2}{c}{}		&			&
&		&$0.11$		&\multicolumn{2}{c}{}				&$1.6$		&$0.3$\\
\par
33	&IRAS~15556		&\multicolumn{2}{c}{}		&			&
&		&		&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{}\\
\par
34	&IRAS~16230		&\multicolumn{2}{c}{}		&			&
&		&$0.06$		&\multicolumn{2}{c}{}				&$6.0$		&$1.2$\\
\par
35	&IRAS~17038		&\multicolumn{2}{c}{}		&			&
&		&$-0.36$	&\multicolumn{2}{c}{}				&$4.6$		&$1.0$\\
\par
36	&IRAS~17233		&\multicolumn{2}{c}{}		&			&
&		&$0.05$		&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{$< $9.4}\\
\par
37	&IRAS~17243		&\multicolumn{2}{c}{}		&			&
&		&$0.07$		&\multicolumn{2}{c}{}				&$3.9$		&$0.8$\\
\par
38	&89~Her		&$1.02$		&$0.59$		&$621$--$980$--$2326$	&$1.38$--$3.45$--$19.43$
&$70$		&$0.09$		&$1.8$		&$1.2$				&$0.7$		&$0.2$\\
\par
39	&AI~Sco		&\multicolumn{2}{c}{}		&			&
&$71.0$		&$-0.24$	&$2.5$		&$1.7$				&$1.9$		&$0.7$\\
\par
40	&IRAS~18123		&\multicolumn{2}{c}{}		&			&
&		&$-0.24$	&\multicolumn{2}{c}{}				&$5.2$		&$1.1$\\
\par
41	&IRAS~18158		&\multicolumn{2}{c}{}		&			&
&		&$0.08$		&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{$< $10.3}\\
\par
42	&AC~Her		&\multicolumn{2}{c}{}		&			&
&$75.4619$	&$-0.07$	&$2.4$		&$1.6$				&$1.3$		&$0.4$\\
\par
43	&AD~Aql		&\multicolumn{2}{c}{}		&			&
&$65.4$		&$0.06$		&$1.7$		&$1.1$				&$4.5$		&$1.5$\\
\par
44	&IRAS~19125		&\multicolumn{2}{c}{}		&			&
&		&$0.09$		&\multicolumn{2}{c}{}				&$1.9$		&$0.4$\\
\par
45	&EP~Lyr		&\multicolumn{2}{c}{}		&			&
&$83.315$	&$0.11$ 	&$2.3$		&$1.6$				&$3.2$		&$1.1$\\
\par
46	&IRAS~19157		&\multicolumn{2}{c}{}		&			&
&		&$0.09$		&\multicolumn{2}{c}{}				&$4.2$		&$0.9$\\
\par
47	&IRAS~20056		&\multicolumn{2}{c}{}		&			&
&		&$-0.03$	&\multicolumn{2}{c}{}				&\multicolumn{2}{c}{$< $9.8}\\
\par
48	&R~Sge			&\multicolumn{2}{c}{}		&			&
&$70.594$	&$0.00$		&$2.0$		&$1.4$				&$1.8$		&$0.6$\\
\par
49	&V~Vul			&\multicolumn{2}{c}{}		&			&
&$75.72$	&$-0.15$	&$2.6$		&$1.8$				&$2.0$		&$0.7$\\
\par
50	&HD~213985		&\multicolumn{2}{c}{}		&			&
&		&$0.04$		&\multicolumn{2}{c}{}				&$3.6$		&$0.7$\\
\par
51	&BD$+$39$^{\circ}$4926	&\multicolumn{2}{c}{}		&			&
&		&$0.11$		&\multicolumn{2}{c}{}				&$4.8$		&$1.0$\\\hline
\end{tabular}
$$
\end{table*}