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\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),
$-\log(L_{\rm x}/L_{\rm bol})$} 
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\begin{tabular}{ccccccccccc}
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\hline
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\#$^{\rm a)}$ & 
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$^{-1}$ &  \\
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\hline
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%       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 \\
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\begin{table*}
\caption[]{ (continued)}
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\begin{tabular}{ccccccccccc}
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\hline
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\#$^{\rm a)}$ &
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$^{-1}$   \\
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\hline
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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 \\
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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*}

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