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Table 2

Parameters of the radiative transfer model grid used to generate a synthetic population of post-AGB disks.

Parameters IRAS 08544-4431 AC Her
Stellar properties

Teff (K) 7250 ± 250 5800 ± 250
logg (dex) 1.5 ± 0.5 1.0 ± 0.5
Z (dex) −0.3 ± 0.3 −1.4 ± 0.3
E(BV) (mag) 1.32 0.46
L* (L) (1.4 104 (2.4 ± 0.2) × 103

Disk parameters

Best fit Grid Best fit Grid

Mdust (M) 2 × 10−3 [2 × 10−4, 2 × 10−3, 2 × 10−2] 2.5 × 10−3 [2.5 × 10−4, 2.5 × 10−3, 2.5 × 10−2]
Rin (au) 8.25 [6.60, 7.43, 8.25, 9.08, 9.90] 34 [27.2, 34.0, 40.8]
3 [2, 2.5, 3] 2.5 [2, 2.5, 3]
Rout (au) 200 200
amin (μm) 0.1 0.01
amax (mm) 1 [1, 10] 1 [1, 10]
pin −1.5 [−2.5, −1.5, −0.5] −3 [−4, −3, −2]
i (°) 19 [0, 35, 50, 64, 75] 50 [0, 35, 50, 64, 75]
q 2.75 [2.2, 2.75, 3.3] 3.25 [2.6, 3.25, 3.9]
αturb 0.01 0.01

Notes. The models are based on the best fit models of IRAS 08544-4431 (Kluska et al. 2018), representing full disks, and AC Her (Hillen et al. 2015), representative of transition disks.

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