Brown dwarf disks with Herschel: Linking far-infrared and (sub)-mm fluxes

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Table 4

Model parameters.

	log(M_disk)	H_p (10AU)	ξ	R_out	H_p (100AU)^b
Model^a	[M_⊙]	[AU]		[AU]	[AU]


BD

mod1a	−4.5	1.5	1.35	50	33.6
mod1b	−4.5	0.15	1.25	50	2.7
mod1c	−4.5	0.15	1.10	50	2.0
mod2a	−3.5	1.5	1.35	50	33.6
mod2b	−3.5	0.15	1.25	50	2.7
mod2b¹	−3.5	0.15	1.25	50	2.7
mod2b²	−3.5	0.15	1.25	50	2.7
mod2b, small	−3.5	0.15	1.25	30	2.7
mod2b, large	−3.5	0.15	1.25	100	2.7
mod2c	−3.5	0.15	1.10	50	2.0
mod3a	−2.5	1.5	1.35	50	33.6
mod3b	−2.5	0.15	1.25	50	2.7
mod3c	−2.5	0.15	1.10	50	2.0


TTS
mod2a	−3.5	1.5	1.35	100	33.6
mod2b	−3.5	0.15	1.25	100	2.7
mod2c	−3.5	0.15	1.10	100	2.0
mod3a	−2.5	1.5	1.35	100	33.6
mod3b	−2.5	0.15	1.25	100	2.7
mod3c	−2.5	0.15	1.10	100	2.0
mod4a	−1.8	1.5	1.35	100	33.6
mod4b	−1.8	0.15	1.25	100	2.7
mod4c	−1.8	0.15	1.10	100	2.0

Notes.

^(a)

mod2b¹ and mod2b² are computed with different grain size distribution: in the first case a_max = 2.4 cm (κ_ν = 2.5 cm² g^-1 at 1300 μm, 14 cm² g^-1 at 160 μm, and 56 cm² g^-1 at 1 μm), in the second a_max = 1.5 μm (κ_ν = 1.5 cm² g^-1 at 1300 μm, 94 cm² g^-1 at 160 μm, and 4.5 × 10³ cm² g^-1 at 1 μm).

^(b)

Scale heights of the disk profile at R = 100 AU as a reference for comparison with previous studies.

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