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Table C.1
Notations used in this study.
| Notations | Units | Explanation |
|
|
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| L ⋆ | [L⊙] | Stellar luminosity |
| M ⋆ | [M⊙] | Stellar mass |
| R ⋆ | [R⊙] | Stellar radius |
| T ⋆ | [K] | Stellar effective temperature |
| d ⋆ | [pc] | Stellar distance |
| i | [°] | Inclination of the disk |
| φ | [°] | Position angle of the disk (disk aligned North-South for φ = 0°, front side is towards the East) |
| r 0 | [au] | Semi latus rectum, the semi-major axis of the disk being r0/ (1−e2) |
| e | Eccentricity of the disk | |
| η | Dust density damping factor | |
| Φe | [°] | Reference angle to define the pericenter (along the semi-major
axis, at the southern side for Φe = φ = 0°) |
| Φη | [°] | Reference angle for the peak density (along the semi-major
axis, at the southern side for Φη = φ = 0°) |
| w | [°] | Width of the Gaussian profile for the azimuthal dust density variation |
| g | Asymmetry parameter for the HG phase function | |
| α in | Slope for the inner dust density distribution | |
| α out | Slope for the outer dust density distribution | |
| ψ | [rad] | Opening angle of the disk |
| β | Radiation pressure to gravitational forces ratio | |
| s blow | [μm] | Dust grain size for which β = 0.5 |
| s min | [μm] | Minimum grain size used in the model |
| s max | [mm] | Maximum grain size |
| p | – | Grain size distribution exponent |
| f 1300 | [mJy] | Flux at 1.3 mm |
| f ice | Fraction of water ice mixed to the dust opacity | |
| f porosity | Fraction of vacuum mixed to the dust opacity | |
| M dust | [M⊕] | Dust mass |
| f ADI | [arbitrary] | Scaling factor for the ADI images |
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