PRODIGE – Planet-forming disks in Taurus with NOEMA - II. Modeling the CO (2–1) isotopologue emission of the Class II T Tauri disks in Taurus

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Table 2

Best fit of the disk physical parameters, compared with the mass estimates from other methodologies, as is discussed in the text.

Source	r_c	T_{atm, 100}	T_{mid, 100}	M_disk	M_dust × 100⁽¹⁾	M_WB⁽²⁾
	(au)	(K)	(K)	(10⁻² × M_⊙)	(10⁻² × M_⊙)	(10⁻² × M_⊙)
CI Tau	150	35	32	2.0	1.6	0.3
CY Tau	40	22	18	1.8	1.9	0.1
DL Tau	125	24	20	2.5	2.5	0.005
DM Tau	200	31	21	4.0	2.5	0.09
DN Tau	40	27	20	2.0	1.3	−
IQ Tau	50	27	19	0.5	0.9	0.007

References.⁽¹⁾ Guilloteau et al. (2011, 2016); Güdel et al. (2018),⁽²⁾ Williams & Best (2014).

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