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Table 1:

Parameters of the Herbig Ae model series.
Quantity Symbol Value
stellar mass $M_\star$ $2.2~M_\odot$
effective temperature $T_{\rm eff}$ 8500 K
stellar luminosity $L_\star$ $32~L_\odot$
disk mass $M_{\rm disk}$ $2.2 \times 10^{-2}$, 10-2,
    10-3, 10-4, 10-5,
    $10^{-6}~M_\odot$
inner disk radius $R_{\rm in}$ 0.5 AU1
outer disk radius $R_{\rm out}$ 700 AU
radial column density power index $\epsilon$ 1.0
dust-to-gas mass ratio $\rho_d/\rho$ 0.01
minimum dust particle radius ${a_{\rm min}}$ $0.05~\mu$m
maximum dust particle radius ${a_{\rm max}}$ $200~\mu$m
dust size distribution power index ${a_{\rm pow}}$ 3.5
dust material mass density $\rho_{\rm gr}$ 2.5 g cm-3
     
strength of incident ISM UV $\chi^{\rm ISM}$ 1
cosmic ray ionization rate of H2 $\zeta_{\rm CR}$ $5\times 10^{-17}$ s-1
abundance of PAHs relative to ISM $f_{\rm PAH}$ 0.1
$\alpha$ viscosity parameter $\alpha$ 0.0

Notes. (1) Soft inner edge applied, see Sect. 3.1 of Woitke et al. (2009a).


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