Shaping the CO snowline in protoplanetary disks | Astronomy & Astrophysics (A&A)

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Table 3

Summary of the dust disk models.

Disk model	# bins in RADMC3D	# bins in NMGC	Grain sizes (µm)	Mass fraction (%)	Opacity
model S	1	1	0.02	100	D_small

model D	2	2	0.02	4.50	D
			10.4	95.5

model C	2	1	0.02	100	D

model M16	16	^(†)	[0.007–651]^(*)	[0.10–32]^(*)	M16

Notes. The grain sizes in Col. 4 and the mass fraction in Col. 5 were calculated using Eqs. (11) and (12), respectively. ^(*)The values are given in Table 4. ^(†)No chemistry computed.

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