Table 2: Disc mass in FUor models: column density $\Sigma$ at 1 and 10 AU from the star, cumulated disc mass ${M_{\rm d}}$ within 10 and 100 AU, and radius ${R_{\rm g}}$ at which the disc's vertical gravity field equals that of the star. Masses are lower values and radii ${R_{\rm g}}$ upper values, obtained with a high viscosity parameter $\alpha = 0.1$ .
$\Sigma$ ( $10^3~{\rm kg}~{{\rm m}}^{-2}$ ) ${{{M_{\rm d}}} ({M_\odot})}$ ${R_{\rm g}}$ (AU)

1 AU 10 AU 10 AU 100 AU

FU Ori 21 4 0.020 0.54 29

V1057 Cyg 15 3 0.015 0.32 50

V1515 Cyg 10 2 0.010 0.24 61

Z CMa B 11 2 0.012 0.31 40

**Table 2:** Disc mass in FUor models: column density $\Sigma$ at 1 and 10 AU from the star, cumulated disc mass ${M_{\rm d}}$ within 10 and 100 AU, and radius ${R_{\rm g}}$ at which the disc's vertical gravity field equals that of the star. Masses are lower values and radii ${R_{\rm g}}$ upper values, obtained with a high viscosity parameter $\alpha = 0.1$ .
	$\Sigma$ ( $10^3~{\rm kg}~{{\rm m}}^{-2}$ )	${{{M_{\rm d}}} ({M_\odot})}$	${R_{\rm g}}$ (AU)
	1 AU	10 AU	10 AU	100 AU
FU Ori	21	4	0.020	0.54	29
V1057 Cyg	15	3	0.015	0.32	50
V1515 Cyg	10	2	0.010	0.24	61
Z CMa B	11	2	0.012	0.31	40

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