\begin{table}%t4 \caption{\label{tab4}Central star magnitude, temperature and luminosity.} \small%\centering \par \begin{tabular}{l c c c c c c c c c c c c c} \hline \hline\noalign{\smallskip} PNe & $m_{V}$ & C & Ref. & $T_{\rm Z}$(H) &$T_{\rm Z}$(HeII) &$T_{\rm EB}$ &$T_{\rm eff}$ &H$\beta$ & dist & $R_{\rm S}$/$R_{\odot}$ & &$L_{\rm S}$/$L_{\odot}$& \\ & meas. & (3) & (4) & (5) & (6) & (7) & (8) & $\times$10$^{11}$ & kpc & (11) & (12) & (13) & (14) \\ \hline BD+30 & 10.28 & 0.50 & 9 & 31~500 & & 30~000 & 30~000 & 29.5 & 1.0 & 1.66 & 1870 & 2450 & \\ Hb~5 & 17.1 & 1.60 & 8 & 105~000 & 130~000 & 145~000 & 140~000 & 11.9 & 2.3 & 0.128 & 5600 & 2700 & 4550 \\ He~2-111 & & & & & & & 200~000: & 1.34 & 2.5 & & & & 650 \\ Hu~1-2 & 17.76 & 0.60 & 6 & 100~000 & 145~000 & 130~000 & 140~000 & 2.22 & 1.5 & 0.0335 & 390 & 210 & 540 \\ IC~418 & 10.23 & 0.33 & 1 & 34~000 & & 36~000 & 35~000 & 58.3 & 1.0 &1.3 & 1850 & 3700 & \\ IC~2165 & 17.47 & 0.59 & 2 & 132~00 & 135~000 & 120~000 & 134~000 & 4.98 & 1.5 & 0.0774 & 1750 & 1810 & 2680 \\ IC~4191 & 16.4 & 0.48 & 11 & 79~000 & 90~000 & 97~000 & 90~000 & 5.25 & 2.1 & 0.099 & 580 & 750 & 1300 \\ M~1-42 & 17.4 & 0.63 & h & 63~000 & 81~000 & 100~000 & 85~000 & 1.0 & 5.0 & 0.179 & 1500 & 810 & 1690 \\ Me~2-1 & 18.40 & 0.28 & 2 & 130~000 & 145~000 & 142~000 & 145~000 & 0.935 & 2.3 & 0.0273 & 300 & 210 & 480 \\ Mz~3 & & 1.65. & & & & & 39~500 & 29.6 & 1.3 & & & 2300 & \\ NGC~40 & 11.55 & 0.605 & 1 & 35~000 & & 40~000 & 38~000 & 17.3 & 0.8 & 0.683 & 875 & 570 & \\ NGC~2022 & 15.75 & 0.38 & 1~11 & 59~000 & 108~000 & 105~000 & 108~000 & 1.79 & 1.8 & 0.099 & 1200 & 220 & 1500 \\ NGC~2440 & 17.63 & 0.50 & 2 & 208~000 & 205~000 & 180~00 & 200~000 & 9.1 & 2.0 & 0.037 & 2000 & 1900 & 2100 \\ NGC~5315 & 14.3 & 0.54 & 3 & 65~000 & 76~000 & 66~000 & 70~000 & 13.3 & 2.0 & 0.306 & 2020 & 1720 & \\ NGC~5882 & 13.42 & 0.33 & 1 & 50~000 & 64~000 & 70~000 & 67~000 & 12.7 & 1.2 & 0.231 & 979 & 590 & 1070 \\ NGC~6153 & 15.55 & 1.14 & 1 & 77~000 & 87~000 & 80~000 & 82~000 & 21.5 & 1.2 & 0.169 & 1200 & 1000 & 2000 \\ NGC~6302 & & & & & & 300~000: & 300.000: & 56. & 1.6 & & & 8000 & 7400 \\ NGC~6445 & 18.72 & 1.06: & 3 & 185~000 & 175~000 & 175~000 & 180~000 & 8.7 & 1.8 & 0.0348 & 1200 & 1380 & 1170 \\ NGC~6537 & 21.6 & 1.79 & 5 & 410~000 & 350~000 & & 350~000: & 12.8 & 2.0 & 0.0147 & 2950 & 4200 & 3700 \\ NGC~6543 & 11.29 & 0.10 & 1 & 47~000 & & 58~000 & 56~000 & 30.8 & 1.0 & 0.457 & 1840 & 1050 & \\ NGC~6741 & 20.09 & 1.1 & 4 & 205~000 & 219~000 & 230~000 & 220~000 & 4.1 & 1.9 & 0.184 & 710 & 850 & 400 \\ NGC~6818 & 17.02 & 0.35 & 3 & 140~000 & 155~000 & 138~000 & 145~000 & 7.43 & 2.0 & 0.048 & 940 & 1270 & 2150 \\ NGC~6886 & 18.76 & 0.70 & 6 & 145~000 & 145~000 & 156~000 & 152~000 & 2.34 & 2.6 & 0.038 & 680 & 670 & 690 \\ NGC~7027 & 16.07 & 1.3 & 2~10 & 165~000 & 160~000 & 234~000 & 180~000 & 134. & 0.9 & 0.0716 & 4820 & 5300 & 4100 \\ NGC~7662 & 14.00 & 0.18 & 1 & 80~000 & 108~000 & 95~000 & 103~000 & 15.3 & 1.2 & 0.118 & 1400 & 770 & 2500 \\ IC~2448 & 14.26 & 0.27 & 1 & 48~000 & 83~000 & 91~400 & 85~000 & 2.35 & 1.4 & 0.147 & 1160 & 151 & 850 \\ NGC~2392 & 10.63 & 0.22 & 1 & 37~000 & 78~000 & 80~000 & 80~000 & 6.83 & 1.5 & 0.845 & 26000 & 490 & 4450 \\ NGC~6826 & 10.68 & 0.07 & 1 & 34~000 & & 45~000 & 42~000 & 12.8 & 1.4 & 0.98 & 2680 & 1120 & \\ NGC~3242 & 12.32 & 0.12 & 12 & 57~000 & 90~000 & 70~000 & 80~000 & 21.4 & 0.55 & 0.14 & 740 & 260 & 1600 \\ NGC~6369 & 15.91 & 2.12 & 3~12 & 69~000 & 71~000 & 70~000 & 70~000 & 61.6 & 1.2 & 0.40 & 3250 & 2850 & 2900 \\ NGC~6210 & 12.66 & 0.14 & 7 & 51~000 & 61~000 & 69~000 & 65~000 & 11.0 & 1.57 & 0.36 & 2070 & 890 & 1060 \\ NGC~2792 & 16.89 & 0.80 & 1~11 & 82~000 & 135~000 & 126~000 & 130~000 & 3.05 & 1.9 & 0.079 & 1600 & 430 & 1570 \\ NGC~1535 & 12.11 & 0.08 & 1 & 40~000 & 76~000 & 87~000 & 80~000 & 4.8 & 2.1 & 0.519 & 9900 & 680 & 2500 \\ \hline \end{tabular} \tablefoot{H$\beta$ in units erg cm$^{-2}$ s$^{-1}$, Col.~7 is the energy balance temperature, Col.~8 is the effective temperature, Col.~12 1s the luminosity found from the magnitude and effective temperature of the central star, Col.~13 is the luminosity found from the nebular hydrogen line, Col.~14 is the luminosity found fron the nebulae ionized helium line. \tablebib{1)~Ciardullo et~al. (\cite{ciar}); 2)~Wolff et~al. (\cite{wolff}); 3)~Gathier \& Pottasch (\cite{gathier}); 4)~Sabbadin et~al. (\cite{sabbadin}); 5)~Matsuura et~al. (\cite{mats}); 6)~Heap et~al. (\cite{heapc}); 7)~Pottasch et~al. (\cite{pbsr}); 8)~Tylenda et~al. (\cite{tylenda}); 9)~Crowther et~al. (\cite{crowther}); 10)~Zijlstra et~al. (\cite{zijlstra}); 11)~Preite-Martinez et~al. (\cite{pmak}); 12)~Pottasch \& Bernard-Salas (\cite{pobs}).}} \vspace*{-4mm} \end{table}