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Table 9

Main results for the 18 old novae.

Object E B − V α (CCM) α (SM)
V603 Aql 0.08 ± 0.02 2.07 ± 0.05 2.01 ± 0.04 17.86 17.43 17.08 17.20 11.50 ± 0.10 11.45 ± 0.11 11.7 ± 0.1
T Aur 0.42 ± 0.08 2.73 ± 0.25 2.39 ± 0.16 2.51 2.52 2.38 2.37 15.45 ± 0.36 15.10 ± 0.46 15.2 ± 0.3
Q Cyg 0.26 ± 0.06 1.20 ± 0.20 1.02 ± 0.15 0.73 0.73 0.71 0.71 14.48 ± 0.28 14.31 ± 0.31 14.9 ± 0.6
HR Del 0.17 ± 0.02 2.31 ± 0.05 2.20 ± 0.04 23.86 23.70 23.25 23.20 11.72 ± 0.11 11.61 ± 0.12 12.1 ± 0.1
DN Gem 0.17 ± 0.04 1.74 ± 0.09 1.65 ± 0.07 0.52 0.53 0.52 0.52 15.18 ± 0.21 15.09 ± 0.24 15.5 ± 0.5
DQ Her 0.05 ± 0.02 0.35 ± 0.06 0.32 ± 0.05 0.22 0.28 0.22 0.28 14.18 ± 0.09 14.16 ± 0.10 14.3 ± 0.3
V446 Her 0.38 ± 0.04 2.07 ± 0.12 1.78 ± 0.09 0.22 0.24 0.23 0.23 17.17 ± 0.18 16.87 ± 0.22 16.9 ± 0.8
V533 Her 0.03 ± 0.02 1.36 ± 0.05 1.35 ± 0.04 0.70 0.68 0.68 0.68 14.02 ± 0.10 14.00 ± 0.11 14.5 ± 0.5
CP Lac 0.28 ± 0.06 1.74 ± 0.14 1.58 ± 0.10 0.64 0.72 0.62 0.70 15.30 ± 0.35 15.14 ± 0.38 15.5 ± 0.3
DI Lac 0.26 ± 0.04 2.00 ± 0.10 1.84 ± 0.08 1.69 1.64 1.58 1.57 14.54 ± 0.21 14.38 ± 0.24 14.7 ± 0.3
DK Lac 0.22 ± 0.06 2.18 ± 0.14 2.05 ± 0.09 0.24 0.26 0.23 0.25 16.72 ± 0.35 16.60 ± 0.38 16.8 ± 0.4
HR Lyr 0.18 ± 0.06 1.15 ± 0.14 1.06 ± 0.10 0.30 0.30 0.30 0.30 15.13 ± 0.35 15.04 ± 0.38 15.5 ± 0.3
BT Mon 0.24 ± 0.06 1.33 ± 0.18 1.17 ± 0.14 0.25 0.29 0.27 0.28 15.74 ± 0.30 15.56 ± 0.34 15.8 ± 0.6
GI Mon 0.10 ± 0.04 1.43 ± 0.08 1.38 ± 0.06 0.20 0.19 0.18 0.18 15.65 ± 0.24 15.60 ± 0.27 15.8 ± 0.8
V841 Oph 0.44 ± 0.06 2.88 ± 0.17 2.55 ± 0.11 13.04 12.97 12.20 12.07 13.92 ± 0.30 13.58 ± 0.36 13.5 ± 0.3
GK Per 0.34 ± 0.04 0.12 ± 0.01 0.11 ± 0.01 1.18 1.19 1.20 1.17 13.09 ± 0.02 13.09 ± 0.02 13.4 ± 0.4
RR Pic 0.00 ± 0.02 1.67 ± 0.04 1.67 ± 0.03 7.26 7.24 7.26 7.23 11.72 ± 0.12 11.72 ± 0.13 12.0 ± 0.2
CP Pup 0.20 ± 0.04 1.59 ± 0.09 1.48 ± 0.07 1.02 0.98 0.96 0.96 14.39 ± 0.21 14.27 ± 0.24 15.0 ± 0.5

Notes.From left to right: the color excess EB − V, the index α of the power-law approximation of the CCM (Cardelli et al. 1989a,b) reddening corrected SED, the same for the SM (Savage & Mathis 1979) reddening corrected SED, the λ-integrated UV flux (in 10-10 erg cm-2 s-1) for the CCM power-law approximation, the CCM dereddened spectral distribution, the SM power-law approximation, and the SM dereddened spectral distribution, respectively. The last three columns give, respectively, the expected observed V-magnitude from the extrapolation of the CCM UV power law after reddening for the visual extinction AV = 3.10 × EB − V, the same from the extrapolation of the SM UV power law, and, finally, the observed visual magnitude.

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