Table 5.
Mean values and ranges of parameters of all photometrically accepted models (Cols. 3–5) and those in spin equilibrium with Pspin = 3484 s (Cols. 6–8; see text for explanation).
| # | Quantity | Photometrically accepted | L2-limited | |||
|---|---|---|---|---|---|---|
| Mean | Sigma | Range | Mean | Sigma | ||
| 1 | d (pc) | 1755 | 284 | 1270–2500 | 1596 | 208 |
| 2 | EB − V (mag) | 0.54 | 0.10 | 0.38–0.70 | 0.58 | 0.09 |
| 3 | (r − i)P1 (mag) | 0.48 | 0.07 | 0.36–0.60 | 0.45 | 0.07 |
| 4 | M2 (M⊙) | 0.41 | 0.20 | 0.16–1.00 | 0.32 | 0.14 |
| 5 | R2 = RRoche (R⊙) | 0.73 | 0.12 | 0.54–1.00 | 0.67 | 0.09 |
| 6 | f3 | 2.03 | 0.61 | 1.02–3.31 | 2.33 | 0.56 |
| 7 | Teff, 2 (K) | 4119 | 143 | 3918–4402 | 4185 | 136 |
| 8 | −log(L2/L⊙) | 0.88 | 0.15 | 1.20–0.47 | 0.92 | 0.15 |
| 9 | M1 (M⊙) | 0.92 | 0.25 | 0.40–1.30 | 0.88 | 0.26 |
| 10 | q = M2/M1 | 0.46 | 0.20 | 0.12–0.85 | 0.38 | 0.18 |
| 11 | i (°) | 77.3 | 2.9 | 72.9–85.7 | 78.4 | 2.9 |
| 12 | a (1011 cm) | 1.64 | 0.16 | 1.24–1.99 | 1.59 | 0.15 |
| 13 | rci/a | 0.13 | 0.03 | 0.10–0.21 | 0.14 | 0.03 |
| 14 | rco/a (Pspin = 3484 s) | 0.20 | 0.01 | 0.19–0.22 | 0.21 | 0.01 |
| 15 | rco/a (Pspin = 3911 s) | 0.22 | 0.01 | 0.20–0.24 | 0.22 | 0.01 |
| 16 | rci/rco (Pspin = 3484 s) | 0.65 | 0.09 | 0.54–0.94 | 0.68 | 0.09 |
| 17 | rci/rco (Pspin = 3911 s) | 0.60 | 0.09 | 0.50–0.87 | 0.63 | 0.09 |
| 18 | Lacc (L⊙)(1) | 2.10 | 0.79 | 0.89–5.53 | 1.95 | 0.75 |
| 19 | Ṁ (10−10 M⊙/yr)(1) | 6.8 | 4.5 | 1.2 –36.9 | 7.0 | 5.0 |
| 20 | Twd (kK) (2) | 27.5 | 5.1 | 14.0–41.3 | 26.3 | 5.0 |
| 21 | Rwd (108 cm)(3) | 6.55 | 2.21 | 3.69–11.86 | 6.93 | 2.23 |
| 22 | rwd (mag)(4) | 23.8 | 0.6 | 22.5–25.2 | 23.7 | 0.6 |
| 23 | gwd (mag)(4) | 23.9 | 0.6 | 22.6–25.4 | 23.8 | 0.6 |
| 24 | μ34 (1034 G cm) | 1.61 | 0.29 | 0.90–2.43 | 1.57 | 0.31 |
| 25 | Bsurf (MG)(5) | 100 | 82 | 7–348 | 85 | 76 |
| 26 | K1 (km s−1) | 96 | 32 | 37–169 | 81 | 27 |
| 27 | K2 (km s−1) | 219 | 34 | 139–299 | 225 | 37 |
Notes. (1) Based on case-B accretion-induced flux; (2) Based on Ṁ in line 19 and Eq. (11); (3) Based on M1, Twd, and WD models with a thick hydrogen envelope (Althaus & Benvenuto 1998; Renedo et al. 2010); (4) Reddened model magnitudes; (5) Based on lines 21 and 24.
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