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Table B.1

DALI model parameters.

Model parameter value Description
Physical structure
rsublrdust cav in 0.4 − 1 au dusty inner disk
δgas cav, δs dust, in, δ1 dust, in 10−5, 10−2, 10−2 surface density drop for rsubl < r < rcav in, dust
rdust cav inrgas cav out 1 − 15 au gas cavity
δgas cav, δs dust cav, δ1 dust cav 10−5, 10−10, 10−10 surface density drop for rdust cav in < r < rgas cav out
rgas cav outrdust cav out 15 − 20 au region outside gas cavity but inside dust cavity
δgas cav edge, δs dust cav edge, δ1 dust cav edge 10−2, 10−2, 10−10 surface density drop for rgas cav out < r < rdust cav out
rgap inrgap out 40 − 175 au gap
δgas gap, δs dust gap, δ1 dust gap 10−1, 10−1, 10−10 surface density drop for rgap in < r < rgap out
r1 dust outrout 250 − 1000 au disk region outside the second ring
δgas out, δs dust oub, δ1 dust out 1, 1, 10−10 surface density drop for rl dust out < r < rout
rc 30 au Characteristic radius of the surface density profile
c 250 g cm−2 Sets the gas surface density at the characteristic radius rc
Mdisk 5 × 10−2 M Mass of the disk
γ 1.1 Power law index of the surface density profile
hc 0.1 Scale height angle at the characteristic radius rc
ψ 0 Flaring index of the disk surface density
PAH abundance 0.1 Gas-phase abundance of PAHs w.r.t. to ISM value
Dust properties
χ 0.2 Settling of large grains
fls 0.85 Mass-fraction of grains that is large
Δgas/dust 100 Gas-to-dust mass ratio
Stellar properties
M* 2.5 M Mass of the central star
L* 36 L Luminosity of the central star
Lx 7.9 × 1028 erg s−1 X-ray luminosity of the central star
Tx 7 × 107 K Effective temperature of the X-ray radiation
ζc.r. 1 × 10−18 s−1 Cosmic ray ionization rate
Observational geometry
i 41° Disk inclination (0° is face-on)
d 108.1 pc Distance to the star
Chemistry(1)
H 5.2 × 10−5
He 1.4 × 10−1
N 3.0 × 10−5
H2 5.0 × 10−1
H2O 1.9 × 10−4
CO 1.3 × 10−4
N2 1.2 × 10−5
NH3 8.1 × 10−6
Mg+ 1.0 × 10−11
Si+ 1.0 × 10−11
S+ 1.0 × 10−11
Fe+ 1.0 × 10−11
tend 5 Myr

Notes. (1) Abundance with regard to the total number of hydrogen atoms. All molecules start as gas-phase species.

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