Table 1
Host stellar properties.
| Name (1) | SpT (2) | Age (Myr) (3) | d (pc) (4) | AV (mag) (5) | L*(L⊙) (6) | Teff (K) (7) | R* (R⊙) (8) | M* (M⊙) (9) | Ṁ (M⊙ yr−1) (10) | Vlsr (km s−1) (11) |
|---|---|---|---|---|---|---|---|---|---|---|
| DL Tau | K7V | 7.8 | 159 ± 1 | 1.6 | 0.37 | 4060 | 1.24 | 0.80 | 5.8 × 10−8 | 6.62 (a) |
| DO Tau | M0V | 2.0 | 139 ± 1 | 3.6 | 0.58 | 3850 | 1.72 | 0.57 | 6.6 × 10−8 | 5.91(b) |
| DR Tau | M0V | 0.9 |  |
2.1 | 1.12 | 3850 | 2.39 | 0.56 | 4.8 × 10−7 | 979 (a) |
| FZ Tau | M0V | 1.1 | 130 ± 1 | 6.5 | 0.93 | 3850 | 2.18 | 0.56 | 3.5 × 10−7 | 6.0 (c) |
| AS 205 A (d) | K5V | 1.1 | 128 ± 2 | 2.9 | 2.14 | 4266 | 2.68 | 0.87 | 4.0 × 10−8 | 4.583 (e) |
| FM Cha (f) | K7V | 5.3 | 201 ± 6 | 4.3 | 0.48 | 4060 | 1.40 | 0.78 | 8.3 × 10−8 | 4.0 (g) |
| WW Cha (h) | K0V | 6.4 | 190 ± 1 | 4.1 | 2.68 | 5110 | 2.09 | 1.65 | 2.1 × 10−7 | 4.3 (g) |
Notes. Columns are defined as: (1) name of the central star, (2) stellar spectral type, (3) stellar age, taken from the evolutionary tracks of Kenyon & Hartmann (1995), (4) distance to the source based on the Gala DR2 supplemental catalog (Bailer-Jones et al. 2018), (5) extinction along the line of sight, (6) stellar luminosity, (7) effective stellar temperature, (8) stellar radius, (9) stellar mass, (10) stellar mass accretion rate, and (11) local standard of rest velocity of the source used in this work, based on literature CO data.
References. All stellar quantities of the sources in Taurus are taken from McClure (2019). (a)Guilloteau et al. (2013). (b)Fernández-López et al. (2020). (c)Taken as the velocity of the maximum [C I] cloud absorption. (d)Andrews et al. (2018). (e)Kurtovic et al. (2018). (f)Manara et al. (2017). (g)Long et al. (2017) and references therein. (h)Manara et al. (2016).
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