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Table 1
Input parameters used in the background disk model.
Parameter | Name | Value | Unit | Reference |
---|---|---|---|---|
M⋆ | Stellar mass | 0.7 | M⊙ | (1) |
L⋆ | Total stellar luminosity | 6 | L⊙ | (2,3) |
Teff | Stellar effective temperature | 4000 | K | (2,3) |
ƒUV | Stellar UV excess | 0.01 | – | (1) |
pUV | UV power law index | 1.3 | – | (1) |
LX | X-ray luminosity | 1 × 1023 | J s−1 | (1) |
TX | X-ray emission temperature | 2 × 107 | K | (1) |
ρm | Monomer material density | 2094 | kg m−3 | (1) |
amin | Minimum background model grain size | 5 × 10−8 | m | (1) |
apow | Background grain size distribution power law slope | 3.5 | – | (1) |
Nbins | Number of grain size bins | 100 | – | (1) |
Mdisk | Disk mass | 0.1 | M⊙ | (3) |
δ | Dust to gas mass ratio | 0.01 | – | (1) |
rin | Inner disk radius | 0.07 | AU | (1) |
rout | Outer disk radius | 600 | AU | (3) |
ϵ | Column density exponent | 1 | – | (1) |
rtaper | Tapering-off radius | 100 | AU | (1) |
H0 | Reference scale height | 10 | AU | (1) |
r0 | Reference scale height radial distance | 100 | AU | (1) |
γ | Disk tapering-off exponent power | 1 | – | (1) |
β | Flaring power | 1.1 | – | (3) |
α | Turbulence strength parameter | 10−3 | – | (3) |
References. (1) Woitke et al. (2016), (2) Siess et al. (2000), (3) this work.
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