Gravitoviscous protoplanetary disks with a dust component - III. Evolution of gas, dust, and pebbles

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Table 1

Model parameters.

Model	M_core	Ω₀	r₀	Σ_g,0	r_out	β
	[M_⊙]	[km s⁻¹ pc⁻¹]	[au]	[g cm⁻²]	[au]	[%]
L	1.03	2.1	1200	0.20	7000	0.24
M	0.53	4.0	617	0.38	3700	0.24
S	0.53	2.2	617	0.38	3700	0.07

Notes. M_core is the initial core mass, Ω₀ and Σ_g,0 are the angular velocity and gas surface density at the center of the core, r₀ is the radius of the central plateau in the initial core, r_out is the initial radius of the core, and β is the ratio of rotational to gravitational energy.

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