Table 1
Main properties of literature sample.
| Target | d | M∗ | log(Ṁacc) | Disk | RALMA |
|---|---|---|---|---|---|
| (pc) | (M⊙) | (M⊙ yr−1) | type | (au) | |
| BP Tau | 127.4 | 0.4 | −8.2 | ⋅ | 41 |
| CIDA 9 | 175.1 | 0.5 | −8.7 | ⊙ | 65 |
| DL Tau | 159.9 | 0.6 | −7.6 | ⊙ | 165 |
| DN Tau | 128.6 | 0.5 | −9.0 | ⊙ | 61 |
| DO Tau | 138.5 | 0.5 | −7.8 | ⋅ | 37 |
| DQ Tau | 195.4 | 0.5+0.5 | −7.7 | ⋅ | 43 |
| DR Tau | 193.0 | 0.4 | −7.9 | ⋅ | 53 |
| DS Tau | 158.4 | 0.5 | −8.6 | ⊙ | 71 |
| FT Tau | 130.2 | 0.3 | −8.9 | ⊙ | 46 |
| GI Tau | 129.4 | 0.7 | −8.4 | ⋅ | 25 |
| GK Tau | 129.1 | 0.9 | −8.7 | ⋅ | 13 |
| GO Tau | 142.4 | 0.4 | −9.1 | ⊙ | 169 |
| HO Tau | 164.5 | 0.3 | −9.1 | ⋅ | 44 |
| HP Tau | 171.2 | 1.7 | −10.6 | ⋅ | 21 |
| HQ Tau | 161.4 | 1.3 | −8.4 | ⋅ | 25 |
| IP Tau | 129.4 | 0.6 | −9.1 | ⊙ | 36 |
| IQ Tau | 131.5 | 0.5 | −8.5 | ⊙ | 110 |
| MWC 480 | 156.2 | 2.1 | −7.6 | ⊙ | 137 |
| UZ Tau E | 123.1 | 0.4+0.3 | −8.0 | ⊙ | 82 |
| V409 Tau | 129.7 | 0.4 | −9.6 | ⋅ | 40 |
| V836 Tau | 167.0 | 0.3 | −8.4 | ⋅ | 31 |
Notes. CIDA 9 can be identified as IRAS 05022+2527 while HP Tau as V* HP Tau. MWC 480 is also known as HD 31648. Columns show target name, distance, stellar mass, mass-accretion rate, disk morphology (· = compact, ⊙ = sub-structured) from 1.3 mm continuum emission (Long et al. 2019), and effective disk radius at 1.3 mm from ALMA. The distance is from Gaia DR3 (Gaia Collaboration 2023); the stellar mass from various sets of pre-main-sequence tracks is from Garufi et al. (2024); the mass-accretion rate is from Gangi et al. (2022), except GO Tau and HO Tau, which are from Ricci et al. (2010); CIDA 9 is from Harsono et al. (2024); and HP Tau from Lin et al. (2023). The ALMA radius is from Long et al. (2019), obtained from their angular measurement of the effective radius encircling 95% of the flux multiplied by the distance from Gaia. The double stellar masses of DQ Tau and UZ Tau E indicate spectroscopic binaries.
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