Table 1: Fundamental parameters of FUor models: accretion rate, inner radius of the disc, flaring H/r, type of dust opacity $\kappa _\lambda$ , and extinction $A_{\rm V}$ .
${M_\star}{\dot{M}}$ ${R_{{\rm min}}}$ H/r $\kappa _\lambda$ $A_{\rm V}$

( ${M_\odot}^2/{\rm yr}$ ) ( ${R_\odot}$ ) (at 10 AU) (Ref.)

FU Ori ${3.2\times10^{-5}}$ 4 0.20 i 1.3

V1057 Cyg ${2.0\times10^{-5}}$ 2 0.35 i 4.5

V1515 Cyg ${1.3\times10^{-5}}$ 5 0.35 h 2.8

Z CMa B ${1.4\times10^{-5}}$ 2 0.20 $^\star$ i 1.8

i: Inhomogeneous aggregates (Henning & Stognienko 1996).

h: Homogeneous aggregates (Henning & Stognienko 1996).

$^\star$ : Not constrained.

**Table 1:** Fundamental parameters of FUor models: accretion rate, inner radius of the disc, flaring H/r, type of dust opacity $\kappa _\lambda$ , and extinction $A_{\rm V}$ .
	${M_\star}{\dot{M}}$	${R_{{\rm min}}}$	H/r	$\kappa _\lambda$	$A_{\rm V}$
	( ${M_\odot}^2/{\rm yr}$ )	( ${R_\odot}$ )	(at 10 AU)	(Ref.)
FU Ori	${3.2\times10^{-5}}$	4	0.20	i	1.3
V1057 Cyg	${2.0\times10^{-5}}$	2	0.35	i	4.5
V1515 Cyg	${1.3\times10^{-5}}$	5	0.35	h	2.8
Z CMa B	${1.4\times10^{-5}}$	2	0.20 $^\star$	i	1.8

Source LaTeX | All tables | In the text

i: Inhomogeneous aggregates (Henning & Stognienko 1996).
h: Homogeneous aggregates (Henning & Stognienko 1996).
$^\star$ : Not constrained.