# Table 2 - The luminosity-specific PN number # for template galaxy models(*) # #---------------------------------------------- # Age M_bol B-V log alpha_03 log alpha_W #[Gyr] #------------------- E ----------------------- 1.0 -23.10 0.66 -7.84 -6.87 2.0 -22.48 0.72 -7.40 -6.56 3.0 -22.13 0.76 -7.16 -6.43 4.0 -21.89 0.79 -6.98 -6.36 5.0 -21.70 0.81 -6.84 -6.32 6.0 -21.54 0.83 -6.73 -6.30 8.0 -21.30 0.86 -6.55 -6.28 10.0 -21.11 0.88 -6.41 -6.27 12.5 -20.92 0.90 -6.29 -6.28 15.0 -20.76 0.92 -6.29 -6.29 # #------------------- Sa --------------------- 1.0 -23.22 0.58 -7.94 -6.98 2.0 -22.67 0.63 -7.51 -6.67 3.0 -22.36 0.65 -7.27 -6.54 4.0 -22.14 0.67 -7.09 -6.47 5.0 -21.97 0.69 -6.95 -6.43 6.0 -21.84 0.70 -6.84 -6.41 8.0 -21.62 0.72 -6.66 -6.38 10.0 -21.45 0.74 -6.53 -6.37 12.5 -21.29 0.75 -6.42 -6.37 15.0 -21.15 0.76 -6.41 -6.38 # #------------------- Sb --------------------- 1.0 -23.11 0.55 -7.99 -7.02 2.0 -22.66 0.58 -7.59 -6.74 3.0 -22.42 0.59 -7.36 -6.63 4.0 -22.25 0.60 -7.20 -6.57 5.0 -22.13 0.61 -7.08 -6.54 6.0 -22.03 0.62 -6.97 -6.52 8.0 -21.88 0.63 -6.81 -6.49 10.0 -21.76 0.63 -6.68 -6.48 12.5 -21.65 0.64 -6.58 -6.48 15.0 -21.57 0.65 -6.57 -6.49 # #------------------- Sc --------------------- 1.0 -22.80 0.55 -7.99 -7.03 2.0 -22.47 0.55 -7.65 -6.80 3.0 -22.34 0.54 -7.46 -6.72 4.0 -22.26 0.54 -7.33 -6.68 5.0 -22.22 0.54 -7.22 -6.66 6.0 -22.19 0.54 -7.14 -6.65 8.0 -22.15 0.54 -7.00 -6.64 10.0 -22.13 0.55 -6.90 -6.63 12.5 -22.12 0.55 -6.81 -6.63 15.0 -22.11 0.56 -6.79 -6.63 # #------------------- Sd --------------------- 1.0 -22.12 0.51 -8.06 -7.09 2.0 -22.05 0.48 -7.80 -6.94 3.0 -22.11 0.46 -7.66 -6.91 4.0 -22.18 0.46 -7.56 -6.89 5.0 -22.25 0.46 -7.48 -6.88 6.0 -22.32 0.46 -7.41 -6.87 8.0 -22.44 0.47 -7.29 -6.84 10.0 -22.54 0.48 -7.19 -6.82 12.5 -22.64 0.49 -7.10 -6.79 15.0 -22.73 0.49 -7.05 -6.77 # #------------------- Im --------------------- 1.0 -20.29 0.30 -9.03 -7.73 2.0 -21.06 0.34 -8.57 -7.55 3.0 -21.49 0.36 -8.31 -7.41 4.0 -21.80 0.38 -8.13 -7.30 5.0 -22.04 0.39 -7.98 -7.21 6.0 -22.24 0.40 -7.86 -7.15 8.0 -22.55 0.42 -7.67 -7.05 10.0 -22.79 0.43 -7.53 -6.99 12.5 -23.03 0.45 -7.39 -6.93 15.0 -23.23 0.46 -7.29 -6.88 #---------------------------------------------- # #(*) Models are for a Salpeter IMF; # # log alpha_03 = luminosity-specific PN number assuming a theoretical # IFMR with a fixed Reimers mass loss parameter \eta = 0.3; # # log alpha_W = luminosity-specific PN number assuming an empirical # IFMR according to Weidemann (2000).