Table 2
Novae assumed distances and best-fit eruption parameters.
| Nova | Distance | Mej | vej | Ṁ w | vw | Dw | tw | f |  |
|---|---|---|---|---|---|---|---|---|---|
| V407 Cyg | 2.7a | 3 × 10−5 | 3000 | 10−4 | 1000 | 10 | 0.5 | 6.25 | 0.73 |
| V1324 Sco | 6.5b | 10−4 | 2000 | 3 × 10−4 | 1000 | 5 | 0.5 | 15.6 | 0.71 |
| V959 Mon | 1.4c | 3 × 10−5 | 3000 | 3 × 10−4 | 1000 | 5 | 1.0 | 1.33 | 0.82 |
| V339 Del | 4.5d | 3 × 10−5 | 1000 | 3 × 10−3 | 1500 | 20 | 2.0 | 0.52 | 0.50 |
| V1369 Cen | 2.5e | 10−4 | 2000 | 10−3 | 1000 | 10 | 2.0 | 0.78 | 0.45 |
| V5668 Sgr | 2.0f | 10−4 | 2000 | 10−3 | 1000 | 20 | 1.0 | 0.18 | 0.32 |
Notes. Distances are given in kpc and the references for them are: (a)Munari et al. (1990); (b)Finzell et al. (2015); (c)Linford et al. (2015); (d)Schaefer et al. (2014); (e)Shore et al. (2014); (f)Banerjee et al. (2016). Cols. 3 to 8 are the best-fit parameters, with the units given in Table 1. Cols. 9 and 10 are the renormalization factors f in the fit to the data and the reduced chi-square of the fit, respectively.
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