Table 1: Accretion disk parameters for FU Ori, for the disk models of KHH, PKHN, LB, and this work. Values marked with an asterisk are assumed.
  $M_{\star}/M_{\odot}$ $\dot{M}/(M_{\odot}/\mbox{yr})$ $M_{\star}\dot{M}/
(M_{\odot}^2/\rm yr)$ $r_{\rm in}/R_{\odot}$ $\cos i$ AV D0/pc
KHH 0.34 $4.36\times10^{-4}$ $1.4\times10^{-4}$ 5.4 0.5* 1.85 500*
PKHN 0.7 $2\times10^{-4}$ $1.4\times10^{-4}$ 5.7 0.5 2.2* 500*
LB 1* $0.82\times10^{-4}$ $0.82\times10^{-4}$ 8 0.65 2* 550*
this work 0.7* $1.4\times10^{-4}$ $1\times10^{-4}$ 11 0.5* 2.2* 500*


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