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Table D.1

Model parameters and values for the reference model.

Quantity Symbol Value
Stellar mass M 0.7, 2.3 M
Effective temperature T 4000, 8600 K
Stellar luminosity L 1, 32 L
UV excess fUV 0.01
UV power-law index pUV 1.3
X-ray luminosity LX 1030 erg/s
X-ray emission temperature TX,fit 2 × 107 K

Strength of interstellar UV χISM 1
Strength of interstellar IR 0
     
Cosmic ray H2 ionization rate ζCR

Disk mass (1) Mdisk 0.01 M
Dust/gas mass ratio (1) δ 0.01
Inner disk radius rin 0.07 AU
Tapering-off radius rtap 100 AU
Column density power index ɛ 1
Rreference scale height Hg(100 AU) 10 AU
Flaring power index β 1.15

Minimum dust particle radius amin 0.05 μm
Maximum dust particle radius amax 3 mm
Dust size dist. power index apow 3.5
Turbulent mixing parameter αsettle 0.01
Max. hollow volume ratio 80%
     
Dust composition Mg0.7Fe0.3SiO3 60%
(volume fractions) amorph. carbon porosity 15%

PAH abundance rel. to ISM fPAH 0.01
Chemical heating efficiency γchem 0.2

Distance d 140 pc
Disk inclination i 45°

12C/13C 70 (150) (2)
18O/16O 540

Thermal over magnetic βmid 102–106
in the midplane

Notes. The meaning of the symbols is explained in Woitke et al. (2009, 2016). (1) The chemical heating efficiency γchem is the efficiency by which exothermic chemical reactions are assumed to heat the gas. A detailed discussion on the disk parameters and their effects on the disk thermal and chemical structure can be found in Woitke et al. (2016). (2) 70 is the adopted standard value (Henkel et al. 1994; Wilson 1999). The choice of 100 corresponds to an average value between the observed ratios by Smith et al. (2015) towards YSOs.

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