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Table 3

Parameters of the PRODIMO disk model used in this paper.

Stellar and irradiation parameters
Stellar mass M* 0.7 M
Stellar luminosity L* 1 L
Eff. temperature T* 4000 K
Excess UV luminosity /L fUV 0.01
UV power law exponent pUV 1.3
X ray luminosity LXray 1(+30)erg s−1
X ray emission temperature TXray 2(+7)K
Interstellar UV field strength χISM 1
Fitting parameter for ζcr ζlow 2(−19)s−1
Fitting parameter for ζcr ζhigh 8(−19)s−1
Fitting parameter for ζcr Σ0 230 cm−2
Fitting parameter for ζcr a −0.01
Disk mass and shape parameters
Disk mass Mdisk 0.01 M⊙
Inner radius Rin 0.07 au
Tapering-off radius (1) Rtap 100 au
Column density exponent ϵ 1.0
Reference radius r0 100 au
Scale height at r0 H0 10.0 au
Flaring power β 1.15
Dust material and size parameters
Dust to gas ratio dust to gas 0.01
Dust composition Mg0.7Fe0.3SiO3 60%
<iPro/> amorph. graphite 15%
porosity 25%
Dust mass density ρgr 2.094 g/cm3
Min. dust radius amin 0.05 μm
Max. dust radius amax 3 mm
Dust size dist. exponent apow 3.5
No. of dust size dist. points Nsize 100
Dust settling parameter αsettle 0.01
Dust parameters for the chemistry
No. of dust size bins Nbin 6
Dust bin fitting indices κ, ζ 1.0, 2.0
Max. dust charge per radius qmax/a 4000 μm−1
Simulation parameters
Grid points in r-direction NXX 500
Grid points in z-direction NZZ 100
Chemical heating efficiency γchem 0.2

Notes. Notation a(b) means a × 10b. (1)The outer radius ROut ≈ 620 au was adjusted automatically to obtain a vertical hydrogen nuclei column density of N〈H〉(ROut) = 1020cm−2.

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