Table 3
Sample of transition disks with dust ring ratios, CO properties, and stellar properties.
| Target | R1 | R2 | Ped.(a) | CO | 12CO | 13CO | Ref. | Class | d | M* | log Macc |
|---|---|---|---|---|---|---|---|---|---|---|---|
| analysis | gap? | gap? | (pc) | (M⊙) | (M⊙ yr−1) | ||||||
| PDS70 | 0.7±0.1 | – | Y | Deep | Y | Y | 1,2 | A | 113 | 0.8 | −10.2 |
| SR21 | 0.7 ± 0.1 | — | M | Deep | Y | Y | 3, 4 | A | 138 | 2.0 | −7.9 |
| HD 169142 | 0.8 ± 0.2 | – | Y | Deep | Y | Y | 5 | A | 114 | 2.0 | −8.7 |
| HPCha | 0.8 ± 0.1 | – | N | – | – | – | – | A | 160 | 1.4 | −9.0 |
| LkCa15 | 0.4 ± 0.2 | 1.2 ± 0.1 | Y | Moderate | M | M | 5 | A/B? | 158 | 0.8 | −8.4 |
| HD 135344B | 0.9 ± 0.2 | 0.7 ± 0.1 | Y | Deep | Y | Y | 3, 6 | A | 136 | 1.6 | −7.4 |
| DoAr44 | 1.0 ± 0.2 | 0.9 ± 0.1 | Y | Deep | – | Y | 3 | A | 146 | 1.0 | −8.2 |
| J16042165 | 1.1 ± 0.3 | 0.8 ± 0.1 | N | Deep | Y | Y | 7, 8 | A | 150 | 1.2 | −10.5 |
| ISO-Oph2 | 1.1 ± 0.1 | – | M | – | N | – | 9 | A/B? | 144 | 0.5 | −8.5 |
| RXJ1633.9 | 1.1 ± 0.1 | – | M | – | Y | – | 9 | A/B? | 141 | 0.8 | −10.0 |
| HD 97048 | 1.2 ± 0.1 | 1.2 ± 0.1 | N | — | Y | Y | 10, 11 | A | 185 | 2.4 | −8.2 |
| SYCha | 1.3 ± 0.0 | – | N | – | N | – | 12 | B | 183 | 0.8 | −9.4 |
| HD 100453 | 1.4 ± 0.2 | – | N | – | N | – | 13 | B | 104 | 1.5 | <−8.3 |
| HD 100546 | 1.4 ± 0.2 | — | N | Deep | Y | Y | 14 | A/B? | 110 | 2.2 | −7.0 |
| SR24S | 1.6 ± 0.2 | 1.3 ± 0.1 | N | – | N | N | 9, 15 | B | 114 | 1.5 | −7.2 |
| GMAur | 1.5 ± 0.2 | 1.4 ± 0.2 | N | Moderate | N | M | 16 | B | 160 | 1.0 | −8.3 |
| J16100501 | 1.8 ± 0.3 | 2.2 ± 0.8 | N | — | — | — | — | B | 145 | 0.6 | −8.6 |
| CSCha | 2.0 ± 0.5 | – | N | – | Y | – | 17 | B | 176 | 1.5 | −8.3 |
| WSB82 | 3.0 ± 0.2 | – | N | – | N | – | 9 | B | 156 | – | – |
Notes. (a)Presence of a pedestal: Y=Yes, N=No, M=Maybe. (1) Muley et al. (2019), (2) Facchini et al. (2021); (3) van der Marel et al. (2016); (4) Yang et al. (2023); (5) Leemker et al. (2022); (6) Casassus et al. (2021); (7) Dong et al. (2017b); (8) Stadler et al. (2023); (9) Antilen et al. (2023); (10) Pinte et al. (2019); (11) Wölfer et al. (2023); (12) Orihara et al. (2023); (13) Rosotti et al. (2020); (14) Leemker et al. (2024); (15) Pinilla et al. (2017); (16) Zhang et al. (2021a); (17) Kurtovic et al. (2022).
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