Table 2
Studied systems, their properties, and the analysed molecules in each case.
| Star(a) | M* [M⊙] | * [L⊙] | Distance [pc] | Inclination [deg] | PA [deg] | Studied molecules(b) |
|---|---|---|---|---|---|---|
| IM Lup | 1.1 | 2.57 | 158 | 47.5 | 144.5 | 12CO, 13CO, C18O, HCN, HCO+, H2CO |
| GM Aur | 1.1 | 1.2 | 159 | 53.2 | 57.2 | 12CO, 13CO, C18O, HCN, HCO+, H2CO |
| AS 209 | 1.2 | 1.41 | 121 | 35.0 | 85.8 | 12CO, 13CO, C18O, HCN, HCO+, H2CO, C2H |
| HD 163296 | 2.0 | 17.0 | 101 | 46.7 | 133.3 | 12CO,13CO, C18O, HCN, CN, HCO+, H2CO, C2H, c-C3H2 |
| MWC 480 | 2.1 | 21.9 | 162 | 37.0 | 148.0 | 12CO, 13CO, C18O, HCN, HCO+, H2CO, C2H |
| Elias 2-27 | 0.46 | 0.91 | 116 | 56.7 | 118.8 | 12CO (2−1), 13CO (3−2), C18O (3−2), CN (7/2−5/2) |
| WaOph 6 | 1.1 | 0.68 | 123 | 47.3 | 174.2 | 12CO (3−2), 12CO (2−1), 13CO (3−2), HCO+ (3−2) |
Notes. (a) Stellar and disk parameters taken from Öberg et al. (2021) for the 5 disks in the MAPS sample and from Huang et al. (2018a) and Andrews et al. (2018) for Elias 2-27 and WaOph 6, except for stellar masses. The stellar mass is estimated dynamically in Veronesi et al. (2021) for Elias 2-27 and in Law et al. (2022) for WaOph 6. (b) The transitions of each molecule for the disks of the MAPS sample are detailed in Sect. 2.1. For Elias 2-27 and WaOph 6 the J transition of each molecule is shown in parenthesis.
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