Table B.1
Observational sample, stellar parameters, and estimated total disk masses
Star | M* | L* | T* | Previous disk mass estimates [M⊙] | References | |||
---|---|---|---|---|---|---|---|---|
[M⊙] | [L⊙] | [K] | Dust mass × 100 | CO flux | HD emission | Dynamical | ||
T Tauri disks | ||||||||
GM Aur | 1.1 | 1.2 | 4350 | 7.3 × 10−2 | 2 × 10−1 | (2.5–20.4) × 10−2 | 1.2 × 10−1 | 1, 13, 16, 18, 20 |
DoAr 25 | 1.06 | 0.95 | 4266 | 4.2 × 10−2 | - | - | - | 4, 3, 5 |
LkCa 15 | 0.7 | 1.098 | 4162 | 2.7 × 10−2 | - | <6.2 × 10−2 | - | 5, 20 |
GW Lup | 0.62 | 0.33 | 3631 | 1.5 × 10−2 | 9.6 × 10−5 | - | - | 4, 3, 12, 5 |
Sz 91 | 0.55 | 0.26 | 3720 | 2.2 × 10−3 | - | - | - | 4, 10, 5 |
DM Tau | 0.50 | 0.24 | 3705 | 1.6 × 10−2 | - | (1.0–4.7) × 10−2 | - | 4, 9, 5, 20 |
Elias 2-27 | 0.46 | 0.91 | 3890 | 3.4 × 10−2 | - | - | 8 × 10−2 | 2, 3, 5, 17 |
Herbig disks | ||||||||
HD 100546 | 2.10 | 23.4 | 9750 | 1.2 × 10−2 | 3.2 × 10−2 | <8 × 10−2 | - | 4, 8, 11, 15, 19 |
HD 97048 | 2.70 | 44.2 | 10500 | 4.7 × 10−2 | 1 × 10−1 | <9.4 × 10−2 | - | 4, 8, 11, 15, 19 |
HD 100453 | 1.66 | 6.31 | 7400 | 5.3 × 10−3 | 3.2 × 10−2 | <1 × 10−2 | - | 6, 11, 15, 19 |
HD 34282 | 1.59 | 13.64 | 8625 | 2.6 × 10−2 | 1.2 × 10−1 | - | - | 7, 11, 15 |
MWC 480 | 2.1 | 21.9 | 8250 | 1.2 × 10−1 | 1 × 10−1 | - | 1.5 × 10−1 | 1, 13, 15, 16 |
HD 163296 | 2.0 | 17.0 | 9332 | 8.4 × 10−2 | 1 × 10−1 | <6.7 × 10−2 | 1.3 × 10−1 | 1, 13, 15, 16, 19 |
HD 142666 | 1.73 | 9.1 | 7500 | 7.6 × 10−3 | 3.2 × 10−2 | - | - | 4, 8, 11, 15 |
Ak Sco | 1.2 | 2.4 | 6250 | 1.8 × 10−3 | 2.3 × 10−3 | - | - | 8, 11, 15 |
References. (1) Öberg et al. 2021 (2) Veronesi et al. 2021 (3) Andrews et al. 2018 (4) Law et al. 2022 (5) Manara et al. 2023 (6) Rosotti et al. 2020 (7) Merín et al. 2004 (8) Fairlamb et al. 2015 (9) Pegues et al. 2020 (10) Tsukagoshi et al. 2019 (11) Stapper et al. 2022 (12) Miotello et al. 2017 (13) Sierra et al. 2021 (14) Brown-Sevilla et al. 2021 (15) Stapper et al. 2024 (16) Martire et al. 2024 (17) Veronesi et al. 2021 (18) Zhang et al. 2021 (19) Kama et al. 2020 (20) McClure et al. 2016
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