Table 1
Stellar properties of all targets in the ALMA-DOT program.
| Target | SpT | Mass (M⊙) | d (pc) | Ref. |
|---|---|---|---|---|
| DG Tau | K7 | 0.3 | 121.2 | a, 1 |
| DG Tau B | – | 1.1 | 140 | b, 2 |
| HL Tau | K3 | 2.1 | 147.3 | c, 3 |
| Haro 6-13 | K5 | 1.0 | 130.4 | d, 1 |
| IRAS 04302+2247 | – | 2.0 | 161 | e, 4 |
| T Tau N, Sa, Sb | K0, –, M | 2, 2, 0.5 | 144.3 | f, 1 |
Notes. Columns are: target name, spectral type, mass, and distance. Spectral types are, when available, from Herczeg & Hillenbrand (2014).
References.References for the mass: a: Isella et al. (2009); b: de Valon et al. (2020); c: Yen et al. (2019); d: Schaefer et al. (2009); e: Guilloteau et al. (2014); f: Köhler et al. (2016). References for the distance: 1: Gaia Collaboration (2018); 2: Garufi et al. (2020); 3: Galli et al. (2018); 4: based on the distance to the parent molecular cloud L1536 (Galli et al. 2019).
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