Multiwavelength analysis for interferometric (sub-)mm observations of protoplanetary disks - Radial constraints on the dust properties and the disk structure

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Table 1

Stellar and disk properties.

Object	SpT	L _⋆	M _⋆	T _⋆	i	PA	Ref.
		(L_⊙)	(M_⊙)	(K)	(°)	(°)

AS 209	K5	1.5	0.9	4250	38	86	1
DR Tau	K7	1.09	0.8	4060	25^a	75^a	2
FT Tau	K6-M3.5^b	0.38	0.85	5000	23	29	3

Notes. For each disk we give the spectral type of the central star, its luminosity, mass, and surface temperature. We also provide the parameters defining the disk geometry, namely the inclination and the position angle (measured east of north).

^(a)

From Eisner et al. (2014);

^(b)

From Luhman et al. (2010a,b).

Reference. (1) Andrews et al. (2009); (2) Ricci et al. (2010b); (3) Guilloteau et al. (2011), Kenyon & Hartmann (1995).

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