\documentstyle{l-aa} % LaTeX A&A Standard Fonts %_____________________________________ \newcommand{\X}{X-ray } \newcommand{\Xs}{X-ray sources } \begin{document} \addtocounter{table}{+5} \begin{table*} \caption[]{Properties of X-ray sources identified with optical stars of known (or assumed) distance. Columns from left to right: running number of Table~2, identified from Table~3 (HD, CPD, CD or DK), V magnitude (from DK), (B-V) colour index (from DK), adopted distance in parsecs, M$_{\rm V}$ inferred absolute visual magnitude, bolometric luminosity , ROSAT X-ray flux in units of 10$^{-14}$ erg cm$^{-2}$ s$^{-1}$, X-ray luminosity $L_{\rm x}$ ($0.16-2.5$ keV), $-\log(L_{\rm x}/L_{\rm bol})$} \begin{flushleft} \begin{tabular}{ccccccccccc} \noalign{\smallskip} \hline \noalign{\smallskip} \#$^{\rm a)}$ & Identification & Sp.$^{\rm b)}$ & V$^{\rm b)}$ & ${\rm (B-V)^{b)}}$ & d & M$_{\rm V}$ & $\log \frac{L}{L_{\sun}}$ & $F_{\rm x}^{\rm c) d)}$ & $L_{\rm x}$ & $-\log \frac{L_{\rm x}}{L_{\rm bol}}$ \\ &HD/CPD/CD/DK & MK & mag & mag & pc & mag & & & erg s$^{-1}$ & \\ \noalign{\smallskip} \hline \noalign{\smallskip} % Iden SP V B-V d Mv L Fx Lx log 1 & CD$-60\degr1889$ & K: & 11.0: & --- &100:& +6: &$-0.4:$& 30$\pm$6 & (3.6:$\pm$1)10$^{29}$ & 3.6 \\ 2 & CPD$-60\degr909$ & K: & 10.5: & --- & 80:& +6:& $-0.4:$& 110$\pm$5 & (9:$\pm$2)10$^{29}$& 3.2 \\ 3 & CPD$-60\degr922$ &Ap-Si\,{\sc ii} & 10.93 & 0.47 & 430 & +2.4 & 0.93:& 12$\pm$2 & (2.7$\pm$0.45)10$^{30}$& 4.1: \\ 4 & 423 & --- & 11.56 & 0.62 & 430 & +3.0 & 0.7 & 3.8$\pm$1.0 & (8.4$\pm$2.2)10$^{29}$& 4.4 \\ 6 & CPD$-60\degr942$ & A1V & 9.97 & 0.16 & 430 & +1.4 & 1.37 & 2.8$\pm$0.8 & (6.2$\pm$1.9)10$^{29}$& 5.2 \\ 7 &CPD$-60\degr944$ A & B9IVp-Si & 8.36 & 0.02 & 430 &$-0.2$& 2.25 & 2.4$\pm$0.7 & (5.3$\pm$1.5)10$^{29}$& 6.1 \\ (7)&CPD$-60\degr944$ B & B9.5IVpSi & 8.78 & 0.09 & 430 & +0.2 & 2.1\\ 8 & 426 & --- & 10.84 & 0.49 & 430 & +2.3 & 0.98 & 4.8$\pm$1.1 & (1.06$\pm$0.24)10$^{30}$& 4.5\\ 10 & 233 & --- & 12.31 & 0.70 & 430 &+3.75 & 0.38 & 3.6$\pm$1.0 & (8.0$\pm$2.2)10$^{29}$& 4.1 \\ 12 & 530 & --- & 12.82 & 0.98 & 190:& +6.1:&$-0.43:$ & 6$\pm$1 & (2.6$\pm$0.4)10$^{29}$& 3.7: \\ \\ 13 &CPD$-60\degr952$ & B9V & 9.29 & 0.12 & 430 & +0.75& 1.66 & 3.8$\pm$1.0 & (8.4$\pm$2.2)10$^{29}$& 5.3 \\ 14 & 412 & --- & 11.27 & 0.65 & 430 & +2.7 & 0.80 & 2.5$\pm$0.8 & (5.5$\pm$1.9)10$^{29}$& 4.6 \\ 16 & 463 & --- & 13.52 & 0.80 & 430 & +5.0&$-0.08$& 2.1$\pm$0.7 & (4.6$\pm$1.5)10$^{29}$& 3.8\\ 17 & 521 & --- & 10.28 & 0.27 & 430 & +1.7 & 1.21 & 4.2$\pm$1.0 & (9.2$\pm$2.2)10$^{29}$& 4.8 \\ 18 & 230 & --- & 12.84 & 0.65 & 430 & +4.3 & 0.20 & 2.7$\pm$0.8 & (6.0:$\pm$1.9)10$^{29}$& 4.0: \\ 19 & CPD$-60\degr961$ & A0IV-V & 8.81 & 0.06 & 430 & +0.25& 1.95 & 2.7$\pm$0.8 & (6.0:$\pm$1.9)10$^{29}$& 5.75 \\ 20 & HD~65\,907 & G0V & 5.61 & 0.57 & 16 & +4.4 & 0.16 & 4.5$\pm$0.6 & (1.4$\pm$0.2)10$^{27}$& 6.15 \\ 23 & 219 & --- & 12.72 & 0.56 & 430 & +4.2 & 0.24 & 3.2$\pm$0.8 & (7.1$\pm$1.9)10$^{29}$ & 4.0 \\ 24 & 403 & --- & 12.88 & 0.79 & 430 & +4.3 & 0.20 & 4.5$\pm$1.0 & (1.0$\pm$0.2)10$^{30}$& 3.8 \\ \\ 26 & 78 & --- & 12.07 & 0.62 & 430 & +3.5 & 0.50 & 3.9$\pm$0.8 & (8.6$\pm$1.9)10$^{29}$ & 4.15 \\ 27 & CPD$-60\degr978$ & A0p-Si & 8.95 & 0.08 & 430 & +0.4 & 1.84 & 1.7:$\pm$0.7& (3.8:$\pm$1.5)10$^{29}$& 5.8:\\ 29 & 206 & --- & 12.78 & 0.60 & 430 & +4.2 & 0.24 & 3.8$\pm$1.0 & (8.4$\pm$2.2)10$^{29}$ &3.9 \\ 31 & CPD$-60\degr981$ & A2Vp-SrCrEu & 9.51 & 0.21 & 430 & +0.95& 1.56 & 3.4$\pm$0.8 & (7.5$\pm$1.9)10$^{29}$& 5.3 \\ 33 & 902 & --- & 11.42 & 0.47 & 430 & +2.9 & 0.72 & 2.9$\pm$0.8 & (6.4$\pm$1.9)10$^{29}$& 4.5 \\ 34 & HD~66\,066 A & B8.5IV & 7.18 & 0.01 & 430 &$-1.4$& 3.16 & 1.8$\pm$0.7 & (4.0$\pm$1.5)10$^{29}$& 7.1 \\ (34)&HD~66\,066 B & B9V & 8.02 & $-0.02$&430&$-0.6$ &2.8\\ 35 & 668 & --- & 14.27 & 0.96 & 430 & +5.7&$-0.38$& 6.7$\pm$1.1 & (1.5$\pm$0.24)10$^{30}$& 3.0 \\ 37 & CPD$-60\degr997$ & A3V & 10.56 & 0.31 & 430 & +2.0 & 1.10 & 2.4$\pm$0.7 & (5.3$\pm$1.5)10$^{29}$& 5.0 \\ 38 & CPD$-60\degr991$ & A0V & 9.72 & 0.11 & 430 & +1.2 & 1.44 & 2.8$\pm$0.8 & (6.2$\pm$1.9)10$^{29}$ & 5.2 \\ \\ 40 & 904 & --- & 12.79 & 0.72 & 430 & +4.2 & 0.24 & 5.3$\pm$1.0 & (1.2$\pm$0.2)10$^{30}$ & 3.7 \\ 41 & 803 & --- & 13.45 & 0.63 & 430 & +4.9&$-0.05$& 4.3$\pm$1.0 & (9.5$\pm$2.2)10$^{29}$ & 3.55 \\ 42 & 86 & --- & 11.70 & 0.61 & 430 & +3.15& 0.62 & 3.2$\pm$0.8 & (7.1$\pm$1.9)10$^{29}$ & 4.35 \\ 43 & 912 & --- & 13.71 & 0.64 & 430 &+5.15&$-0.14$& 4.2$\pm$1.0 & (9.3$\pm$2.2)10$^{29}$ & 3.5 \\ 46 & HD~66\,194 &B2.5IVe & 5.80 &$-0.09$&430 &$-2.75$&3.90 & 8.5$\pm$1.3 & (1.9$\pm$0.3)10$^{30}$ & 7.2 \\ 47 & HD~66\,167 A & A0V & 9.51 & 0.08 & 430 & +0.95& 1.55 &20.3$\pm$2.0 & (4.5$\pm$0.45)10$^{30}$& 4.5 \\ & HD~66\,167 B & B9.5V & 9.56 & 0.16 & 430 & +1.0 & 1.53 & \\ 48 & CPD$-60\degr1008$&A1/2V & 9.77 & 0.18 & 430 & +1.2 & 1.44 & 6.0$\pm$1.3 & (1.3$\pm$0.3)10$^{30}$ & 4.9 \\ 51 & 811 & --- & 11.98 & 0.51 & 430 & +3.4 & 0.52 & 4.9$\pm$1.0 & (1.1$\pm$0.2)10$^{30}$ & 4.1 \\ 52 & HD~66\,295 & A0p-Si & 9.11 & 0.03 & 430 &+0.55 & 1.74 & 4.5$\pm$1.0&(1.0$\pm$0.2)10$^{30}$ &5.3 \\ \noalign{\smallskip} \hline \noalign{\smallskip} \end{tabular} \end{flushleft} \end{table*} %______________________ \addtocounter{table}{-1} %------------------------ \begin{table*} \caption[]{ (continued)} \begin{flushleft} \begin{tabular}{ccccccccccc} \noalign{\smallskip} \hline \noalign{\smallskip} \#$^{\rm a)}$ & Identification & Sp.$^{\rm b)}$ & V$^{\rm b)}$ & ${\rm (B-V)^{b)}}$ & d & M$_{\rm V}$ & $\log \frac{L}{L_{\sun}}$ & $F_{\rm x}^{\rm c) d)}$ & $L_{\rm x}$ & $-\log \frac{L_{\rm x}}{L_{\rm bol}}$ \\ & & MK & mag & mag& pc & mag & && erg s$^{-1}$ \\ \noalign{\smallskip} \hline \noalign{\smallskip} 53 & CPD$-60\degr1016$&---&9.86 & 0.54 & 430:& +1.3:& 1.42:& 3.5:$\pm$1.3&(7.7:$\pm$2.9)10$^{29}$&5.1:\\ 54 & HD~66\,318&A0:p-TiSi& 9.65 & 0.07 & 430 & +1.1 & 1.48 & 2.5$\pm$1.0 &(5.5:$\pm$2.2)10$^{29}$&5.3:\\ 55 & 96 & --- & 13.98 & 0.88 & 430 & +5.4 & $-0.26$ & 4.2$\pm$1.0 & (9.3$\pm$2.2)10$^{29}$ & 3.35 \\ 57 & 879 & --- & 14.67 & 0.83 & 430 & +6.1 & $-0.59$ & 2.5$\pm$0.8 & (5.5$\pm$1.9)10$^{29}$ & 3.25 \\ 61 & 647 & K: & 13.06 & 1.25 & 120:& +7:&$-0.8:$& 19$\pm$2& (2.3:$\pm$0.5)10$^{29}$ & 3.4 \\ 62 & 868 & --- & 13.02 & 0.65 & 430 & +4.5 & 0.12 & 18$\pm$2.1 & (4.0$\pm$0.5)10$^{30}$ & 3.1 \\ \noalign{\smallskip} \hline \noalign{\smallskip} \end{tabular} \end{flushleft} Notes: \\ a) running number in Table~2\\ b) from Dachs \& Kabus (\cite{da:ka}) or from this paper \\ c) in units of $10^{-14}$ erg cm$^{-2}$ s$^{-1}$ \\ d) Adopted flux conversion factor $C_{\rm F}$ for NGC~2516 cluster stars showing HR1 $\approx +1.0$:\\ ~~~$C_{\rm F}\approx 1.4~10^{-11}$ erg cm$^{-2}$ s$^{-1}$ $({\rm ~counts}~{\rm s}^{-1})^{-1}$ \\ \end{table*} \begin{thebibliography}{} \end{document}