Table 9.
Free parameters of best-fit models of β Lyr A.
Slab | Slab | Wedge | Wedge | Nebula | ||||
---|---|---|---|---|---|---|---|---|
Par. | Unit | Min | Max | Power-law | Steady | Power-law | Steady | Power-law |
H | R⊙ | 5.5 | 12 | 6.10 ± 0.78 | 6.84 ± 1.34 | |||
ϑ | deg | 7.5 | 12.75 ± 0.71 | 12.96 ± 0.86 | ||||
Rout | R⊙ | 35 | 30.77 ± 0.75 | 27.71 ± 1.19 | 30.36 ± 0.54 | 30.79 ± 0.55 | 31.11 ± 0.82 | |
T0 | K | 23 000 | 35 000 | 33948 ± 313 | 30 849 ± 740 | 30 292 ± 1026 | ||
T1 | K | 23 000 | 35 000 | 26 995 ± 778 | 26 424 ± 619 | |||
ρ0 | 10−6 g cm−3 | 0.001 | 5.00 | 2.90+1.07 | 4.82+0.17 | 0.99+1.21 | 0.07+1.24 | 3.46 ± 1.01 |
αD | 1 | −4.0 | −0.8 | −0.93 ± 0.58 | −2.43 ± 0.67 | −2.44 ± 0.67 | −3.16 ± 0.68 | −2.40 ± 0.25 |
αT | 1 | −1.2 | −0.7 | −1.03 ± 0.10 | −0.95 ± 0.10 | −1.00 ± 0.10 | ||
i | deg | 91 | 95 | 93.26 ± 0.26 | 92.66 ± 0.51 | 94.11 ± 0.45 | 94.15 ± 0.25 | 93.26 ± 0.26 |
Ω | deg | 252 | 255 | 253.65 ± 0.85 | 253.97 ± 0.75 | 253.40 ± 1.26 | 253.42 ± 0.76 | 253.65 ± 0.85 |
d | pc | 305 | 330 | 316.7 ± 5.7 | 315.9 ± 6.2 | 321.2 ± 3.7 | 321.4 ± 6.5 | 319.7 ± 2.7 |
hinv | H | 1 | 9 | 3.58 ± 0.16 | ||||
tinv | T(r) | 1 | 9 | 8.92 ± 0.30 | ||||
hwind | H | 1 | 15 | 5.32 ± 0.35 | ||||
hmul | H | 1 | 15 | 4.32 ± 0.26 |
Notes. H denotes the geometric semi-thickness, ϑ the half opening angle of the wedge, Rout the outer geometric radius of the disk, T0 the temperature at the inner rim for a power-law radial temperature profile (given by Eq. (8)), T1 the characteristic temperature of the disk, with the maximum temperature Tmax = 0.488 T1 (Eq. (9)), ρ0 the density at the inner rim, αT the exponent of the temperature profile, αD the exponent of the density profile, i the orbital inclination, Ω the longitude of ascending node, and d the distance of the system. “Min” and “Max” denote boundaries of the intervals that were searched by the global-optimization algorithm. The lower bound of the density ρ is not indicated for the wedge and slab models; it can reach down to ∼10−9 g cm−3 while the disk remains optically thick.
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