Table 4: Parameter set for the passive disk model, the active model (Sect. [*]) and the active model with an envelope (Sect. 5.3). Results correspond to Fig. 6.
Parameter Passive disk Active disk Active disk ${\rm +}$ envelope
  model model model
Stellar mass $M_{\star}$ $1.69\ M_{\odot}$ $1.69\ M_{\odot}$ $1.69\ M_{\odot}$
Stellar temperature $T_{\star}$ $5560\ {\rm K}$ $5560\ {\rm K}$ $5560\ {\rm K}$
Stellar luminosity $L_{\star}$ $10.0\ L_{\odot}$ $10.0\ L_{\odot}$ $10.0\ L_{\odot}$
Disk mass $M_{\rm disk}$ $1 \times 10^{-2}\ M_{\odot}$ $4 \times 10^{-3}\ M_{\odot}$ $4 \times 10^{-3}\ M_{\odot}$
Outer disk radius $R_{\rm out}$ $270\ {\rm AU}$ $270\ {\rm AU}$ $270\ {\rm AU}$
Inner disk radius $R_{\rm in}$ $0.3\ {\rm AU}$ $0.3\ {\rm AU}$ $0.3\ {\rm AU}$
Exponent p (see Eq. (2)) 1.3 1.3 1.4
Inclination $\vartheta $ $\lse$ $70^{\circ}$ $\lse$ $70^{\circ}$ $\lse$ $65^{\circ}$
$c_{\rm 1}$ (see Eq. (5)) - - $5.0 \times 10^{-5}$
$c_{\rm 2}$ (see Eq. (5)) - - 1.0
Accretion rate $\dot{M}$ - $9.1 \times 10^{-8}$ $M_{\odot}$ yr-1 $2.5 \times 10^{-8}$ $M_{\odot}$ yr-1
Boundary temperature $T_{\rm bnd}$ - $8000\ {\rm K}$ $8000\ {\rm K}$
Truncation radius $R_{\rm bnd}$ - $5\ R_{\star}$ $5\ R_{\star}$


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