Table 1
Summary of disk parameters used in this work and references.
| Source | M★ (a) [M⊙] | Dust | Gas |
|---|---|---|---|
| TW Hya | 0.6 | (1) | (4) |
| GM Aur | 1.1 | (2) | (5) |
| IML up | 1.1 | (2) | (5) |
| AS 209 | 1.2 | (2) | (5) |
| HL Tau | 1.7 | (3) | (6) |
| HD 163296 | 2.0 | (2) | (5) |
| MWC 480 | 2.1 | (2) | (5) |
Notes. (a) All stellar masses are dynamically determined by disk Keplerian rotation, TW Hya (Teague et al. 2022), HL Tau (Pinte et al. 2016), MAPS sources (Öberg et al. 2021; Teague et al. 2021).
References. (1) Macías et al. (2021); (2) Sierra etal. (2021); (3) Guerra-Alvarado et al. (in prep.); (4) Calahan et al. (2021); (5) Zhang et al. (2021); (6) Booth & Ilee (2020).
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