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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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