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Table A.1
Model parameters for the comparison with Visser et al. (2015).
| Quantity | Symbol | Value |
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| stellar mass | M ∗ | 0.5 M⊙ |
| stellar effective temp. | T ∗ | 5000 K |
| stellar luminosity | L ∗ | 1.6 L⊙ |
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| strength of interst. FUV | χ ISM | 1a |
| cosmic ray H2 ion. rate | ζ CR | 5 × 10-17 s-1 |
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| centrifugal radius | R c | 0 au b |
| mass infall rate | Ṁ if | 2 × 10-5M⊙ yr-1 |
| inner radius | R E,in | 6.2 au |
| outer radius | R E,out | 6200 au |
| cavity opening angle | β cav | 20° |
| dust/gas mass ratio | d / g | 0.01 |
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| min. dust particle radius | a min | 0.005 μm |
| max. dust particle radius | a max | 0.25 μm |
| dust size dist. power index | a pow | 3.5 c |
Notes.
(a)
χISM is given in units of the Draine field (Draine & Bertoldi 1996; Woitke et al. 2009).
(c)
For the dust composition see Table 1
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