PRODIGE – planet-forming disks in Taurus with NOEMA - I. Overview and first results for 12CO, 13CO, and C18O

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Volume 685 (May 2024)

A&A, 685 (2024) A126

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Table 2

Disk properties.

Source	V_LSR (km s⁻¹)	Incl. (°)	PA (°)	R_disk (au)	$M_{disk}^{dust} \times 100$ $M_{{\rm{disk}}}^{{\rm{dust}}} \times 100$ (M_⊙)	S_v (1.3 mm) (mJy)	Age (Myr)	References
CI Tau	5.74	${49.99}_{- 0.12}^{+ 0.11}$ ${49.99_{ - 0.12}^{ + 0.11}}$	${281.22}_{- 0.13}^{+ 0.13}$ ${281.22_{ - 0.13}^{ + 0.13}}$	520 ± 13	0.016	125.3 ± 6.2	${2.5}_{- 1.1}^{+ 2.0}$ ${2.5_{ - 1.1}^{ + 2.0}}$	(1,4,6)
CY Tau	7.25	34 ± 3	63 ± 5	295 ± 11	0.019	111.1 ± 2.9	${2.3}_{- 0.6}^{+ 0.7}$ $2.3_{ - 0.6}^{ + 0.7}$	(1,3)
DG Tau	5.5	32 ± 2	60 ± 4	300± 50	0.036	389.9 ± 4.6	${0.28}_{- 0.08}^{+ 0.12}$ $0.28_{ - 0.08}^{ + 0.12}$	(2,3)
DL Tau	6.10	${44.95}_{- 0.09}^{+ 0.09}$ ${44.95_{ - 0.09}^{ + 0.09}}$	${322.14}_{- 0.14}^{+ 0.15}$ ${322.14_{ - 0.14}^{ + 0.15}}$	463 ± 6	0.025	204.4 ± 1.9	${3.5}_{- 1.6}^{+ 2.8}$ ${3.5_{ - 1.6}^{ + 2.8}}$	(1,4,6)
DM Tau	6.05	−34.7 ± 0.7	64.7 ± 0.2	900 ± 10	0.025	108.5 ± 2.4	1–5	(1,5,7)
DN Tau	6.38	${35.18}_{- 0.22}^{+ 0.2}$ ${35.18_{ - 0.22}^{ + 0.2}}$	${349.19}_{- 0.38}^{+ 0.36}$ ${349.19_{ - 0.38}^{ + 0.36}}$	241 ± 7	0.013	${88.61}_{- 0.2}^{+ 0.09}$ ${88.61_{ - 0.2}^{ + 0.09}}$	${0.9}_{- 0.4}^{+ 0.6}$ ${0.9_{ - 0.4}^{ + 0.6}}$	(1,4,6)
IQ Tau	5.47	58.2 ± 0.2	313.8 ± 0.22	220 ± 15	0.009	${64.11}_{- 0.34}^{+ 0.25}$ ${64.11_{ - 0.34}^{ + 0.25}}$	${4.2}_{- 2.0}^{+ 4.1}$ ${4.2_{ - 2.0}^{ + 4.1}}$	(1,4,6)
UZ Tau E	5.70	56.15 ± 0.07	0.39 ± 0.08	300± 20	0.018	149.9 ± 1.4	${1.3}_{- 0.6}^{+ 1.0}$ ${1.3_{ - 0.6}^{ + 1.0}}$	(1,4,6)

Notes. The systemic velocities, the outer gas radii, and the disk masses measured from the dust emission for all disks but DG Tau are adopted from Guilloteau et al. (2016), and for DG Tau from Güdel et al. (2018) and Guilloteau et al. (2011). The S_v(1.3 mm) continuum fluxes for all disks but IQ and DN Tau are taken from Guilloteau et al. (2016) and for the IQ Tau and DN Tau from Long et al. (2018). The inclination and positional angle (PA) for CI, DL, DN, IQ and UZ Tau E are taken from Long et al. (2018), for DM Tau from Piétu et al. (2007), and for CY and DG Tau from Guilloteau et al. (2011). Position angles are those of the disk rotation axis. The disk ages for CI, DL, DN, IQ Tau and UZ Tau E are taken from Long et al. (2019), for CY and DG Tau from Guilloteau et al. (2011), and for DM Tau from Law et al. (2022).

References: (1) Guilloteau et al. (2016), (2) Güdel et al. (2018), (3) Guilloteau et al. (2011), (4) Long et al. (2018), (5) Piétu et al. (2007), (6) Long et al. (2019), and (7) Law et al. (2022).

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