Variable accretion as a mechanism for brightness variations in T Tauri S

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Table 5:

Summary of the parameters of the radiative transfer model described in Sect. 4.2 and Figs. 5-7.
Parameter	Symbol	Value	Unit
stellar radius	R_*	3.5	$R_{\odot}$
stellar mass	M_*	2.2	$M_{\odot }$
effective temperature	$T_{\rm {eff}}$	5500	K
stellar luminosity	L_*	10	$L_{\odot}$
disk mass	$M_{\rm {disk}}$	10^-3	$M_{\odot }$
exponent surface density	p	-1
inner radius passive disk	$R_{\rm {in}}$	0.5	AU
outer radius passive disk	$R_{\rm {out}}$	5.0	AU
scale height at inner edge	H₀	0.021	AU
flaring index	$\gamma$	2/7
accretion rate	$\dot M_{{\rm acc}}$	10^-8, 10^-6, 10^-5	$M_{\odot }$ yr^-1
inner radius active disk	$R_{\rm {in, SS}}$	0.036	AU
outer radius variable $\dot M_{{\rm acc}}$	$R_{\rm {out, acc}}$	0.5	AU
inclination	i	74	deg
foreground extinction	$A_{\rm V}$	15	mag

Source LaTeX | All tables | In the text

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