Table 1
Source properties of the sample.
| Source | d (pc) | Av (mag) | L* (L⊙) | M* (M⊙) | Vrad(±err) (km s−1) | log Lacc (±err) (L⊙) | log Ṁacc (M⊙ yr−1) | idisk(a) (deg) | Disk type(b) | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|
| BP Tau | 127 | 0.2 | 0.37 | 0.48 | 16.09(0.16) | −1.34 (0.07) | −8.25 | 38.2 ± 0.5 | Sub | 1,2 |
| CI Tau | 160 | 2.6 | 1.04 | 1.29 | 17.06(0.35) | 0.02 (0.06) | -7.28 | 50 ± 0.3 | Sub | 1 |
| CQ Tau | 149 | 0.5 | <15.1 | <1.99 | 24.85(1.15) | < -0.42 | <-7.68 | 32.2-35 | TD | 3,9 |
| CW Tau | 131 | 3.6 | 0.40 | 0.90 | 16.45(1.85) | -0.07 (0.07) | -7.47 | 57.8-59.2 | Full | 4,12 |
| CY Tau | 126 | 0.0 | 0.22 | 0.36 | 16.19(0.43) | -2.00 (0.07) | -8.85 | 28 ± 5 | Full | 5, 10 |
| DE Tau | 128 | 0.0 | 0.49 | 0.26 | 14.67(0.44) | −1.45 (0.08) | −7.99 | - | Full | 6 |
| DF Tau | 176 | 0.0 | 0.35 | 0.39 | 14.8(0.54) | -0.75 (0.06) | -7.55 | 52 | Full | 7 |
| DG Tau | 125 | 1.5 | 0.44 | 0.70 | 14.34(1.89) | -0.25 (0.18) | -7.35 | 37 | Full | 4 |
| DH Tau | 133 | 0.6 | 0.20 | 0.41 | 15.57(0.33) | −1.53 (0.07) | −8.49 | 16.9 ± 2.2 | TD | 1 |
| DK Tau | 132 | 1.2 | 0.78 | 0.62 | 17.31(0.20) | −1.42 (0.07) | −8.33 | 58 ± 18 | Full | 1,11 |
| DL Tau | 160 | 1.5 | 0.40 | 0.90 | 16.56(0.23) | -0.35 (0.18) | -7.62 | 45.0 ± 0.2 | Sub | 1 |
| DN Tau | 129 | 0.5 | 0.49 | 0.55 | 17.44(0.21) | -2.10 (0.09) | -9.04 | 35.2 ± 0.5 | Sub | 1 |
| DO Tau | 138 | 1.4 | 0.42 | 0.50 | 18.81(0.78) | -0.93 (0.11) | -7.80 | 27.6 ± 0.5 | Full | 1 |
| DQ Tau | 195 | 1.5 | 0.98 | 0.52 | 20.86(0.52) | -0.92 (0.07) | -7.68 | 16.1 ± 1.2 | Full | 1 |
| DR Tau | 193 | 1.2 | 0.29 | 0.83 | 22.57(0.26) | -0.56 (0.08) | -7.93 | 5.4 ± 2.6 | Sub | 1 |
| DS Tau | 158 | 0.4 | 0.29 | 0.61 | 15.50(0.32) | −1.46 (0.07) | −8.57 | 65.2 ± 0.3 | Sub | 1 |
| FT Tau | 130 | 0.6 | 0.05 | 0.25 | 16.65(0.79) | −1.93 (0.09) | −8.92 | 35.5 ± 0.3 | Sub | 1 |
| GG Tau | 116 | 1.4 | 0.80 | 0.73 | 17.59(0.34) | -0.76 (0.08) | -7.76 | 54-61 | TD | |
| GH Tau | 130 | 0.8 | 0.79 | 0.42 | 16.98(0.96) | -2.31 (0.09) | -8.98 | - | Full | |
| GI Tau | 129 | 1.9 | 0.27 | 0.55 | 18.64(0.47) | −1.37 (0.07) | −8.43 | 43.8 ± 1.1 | Full | 1 |
| GK Tau | 129 | 1.9 | 0.87 | 1.20 | 20.96(0.32) | −1.39 (0.10) | −8.67 | 40.2 ± 6.0 | Full | 1 |
| GM Aur | 158 | 1.3 | 1.16 | 1.19 | 15.98(0.37) | −1.05 (0.09) | −8.29 | 53.21 | TD | |
| HN Tau | 134 | 1.2 | 2.63 | 1.58 | 27.34(2.25) | -0.12 (0.23) | -7.31 | 69.8 ± 1.4 | Full | 1 |
| HQ Tau | 161 | 3.7 | 5.83 | 2.00 | 17.52(1.05) | −1.24 (0.14) | −8.43 | 53.8 ± 3.2 | Full | 1 |
| IP Tau | 129 | 0.6 | 0.31 | 0.51 | 17.40(0.26) | -2.15 (0.10) | -9.14 | 45.2 ± 0.9 | TD | 1 |
| IQ Tau | 131 | 1.6 | 0.19 | 0.55 | 17.50(0.42) | −1.40 (0.08) | −8.54 | 62.1 ± 0.5 | Sub | 1 |
| LkCa 15 | 157 | 0.9 | 0.60 | 1.09 | 19.43(0.17) | −1.89 (0.09) | −9.24 | 51.5 ± 0.7 | TD | 3,13 |
| MWC480 | 156 | 0.0 | 10.79 | 1.71 | 12.87(1.10) | -0.19 (0.12) | -7.64 | 36.5 ± 0.2 | Sub | 1 |
| RW Aur A | 183 | 1.0 | 1.64 | 1.50 | 27.7(2.5)(c) | +0.39 (0.30) | -6.93 | 55.1 ± 0.5 | TD | 1 |
| RY Tau | 138 | 2.2 | 8.87 | 1.80 | 21.73(1.51) | -0.38 (0.15) | -7.57 | 65.0 ± 0.5 | Sub | 1 |
| UX Tau | 142 | 1.2 | 1.76 | 1.36 | 19.74(0.35) | −1.26 (0.16) | −8.58 | 57-88 | TD | |
| UY Aur A | 152 | 0.5 | 0.46 | 0.51 | 14.09(0.50) | −1.27 (0.07) | −8.18 | 23.5 ± 7.8 | Sub | 1 |
| UZ Tau E | 130 | 0.7 | 0.45 | 0.41 | −0.56(1.31) | −1.27 (0.07) | −8.05 | 56.1 ± 0.5 | Sub | 1 |
| V409 Tau | 130 | 0.3 | 0.24 | 0.43 | 16.98(0.36) | -2.64 (0.13) | -9.58 | 69.3 ± 0.3 | TD | 1 |
| V807 Tau | 184 | 1.3 | 1.69 | 1.41 | 16.75(0.15) | -0.91 (0.09) | -8.14 | - | TD | 8 |
| V836 Tau | 167 | 0.9 | 0.54 | 0.22 | 19.18(0.18) | −1.93 (0.09) | −8.37 | 43.1 ± 0.8 | Full | 1 |
Notes. Stellar and accretion parameters derived from GHOsT data in Gangi et al. (2022) and Alcalá et al. (2021). Average uncertainties are 0.2 in Av, 0.2 in log L*, and 0.15 in log M*. Distances are from Gaia EDR3 with a typical uncertainty <10%. See Gangi et al. (2022) and Alcalá et al. (2021) for details.(a) Inclination angles refer to the outer disk estimated from millimetres observations, except for GG Tau, UX Tau and DK Tau for which an inner disk inclination different from the outer disk was measured outside observational errors (see also Table 3). Errors on the inclination or a range of values is given when available. (b)Disk type refer to the disk structure as revealed by resolved millimetre images, i.e. disks with substructures such as rings and holes (sub), full disks (full) or disks with inner sub-mm dust cavities (TD). (c) Radial velocity for RW Aur derived from the Li line only.
References for disk parameters. (1) Long et al. (2019), (2) Jennings et al. (2022), (3) Francis & van der Marel (2020), (4) Bacciotti et al. (2018), (5) Tripathi et al. (2017), (6) Simon et al. (2019), (7) Andrews et al. (2013), (8) Simon et al. (2016), (9) Bohn et al. (2022), (10) Pérez et al. (2015), (11) Nelissen et al. (2023), (12) Ueda et al. (2022), (13) Piétu et al. (2007).
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