Mid-infrared blends and continuum signatures of dust drift and accretion in protoplanetary disks

Open Access

Table 1

Disk model series used in this study.

Model series	Antonellini et al. (2015)	Greenwood et al. (2019a)
M_gas (M_⊙)	10⁻⁵−10⁻¹	0.1 (initial) (*)
a_pow ⁽−⁾	2.0–1.5	Evolving
β (−)	0.8−1.25	1.15
R_in (au)	0.05–55	0.07

Notes. (*) Due to viscous accretion there is a drop in the gas mass during the disk time evolution, which is up to 50% of the initial value.

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