Table 3
Position of millimeter and scattered light cavities for 22 transition disks, ordered by increasing millimeter cavity size.
| Source | d(pc) | Band | Rpeak,mm (au) | Rin,PI (au) | Rpeak,PI (au) | Ratio | |
|---|---|---|---|---|---|---|---|
| HD 100546 | 110 ± 1 | B7 – R’ | 15.0 | 12.0 | 14.0 | 0.81, 0.96 | |
| HD 169142 | 114 ± 1 | B6 – J | 21.7 | 16.0 | 20.5 | 0.74, 0.94 | |
| V4046Sgr | 72 ± 1 | B6 – H | 27.0 | 15.3 | 26.9 | 0.57, 0.99 | |
| UX Tau A | 140 ± 2 | B6 – H | 33.2 | < | 14 | < 0.42 | |
| HD 100453 | 104 ± 1 | B6 – R’ | 33.3 | 14.6 | 18.5 | 0.44, 0.55 | |
| T Cha | 110 ± 1 | B3 – H | 36.8 | 28.8 | 31.4 | 0.78, 0.85 | |
| HD 143006 | 166 ± 4 | B6 – J | 40.0 | 18.2 | 30.0 | 0.45, 0.75 | |
| DoAr44 | 146 ± 1 | B7 – H | 42.7 | < | 14 | < 0.33 | |
| CQ Tau | 163 ± 2 | B6 – J | 47.3 | < | 4 | < 0.08 | |
| J1852 | 146 ± 1 | B3 – H | 43.8 | 34.7 | 43.1 | 0.79, 0.98 | |
| HD 135344B | 136 ± 2 | B7 – R | 54.6 | 18.3 | 23.5 | 0.34, 0.43 | |
| HD 97048 | 185 ± 1 | B7 – J | 55.4 | 45.9 | 54.4 | 0.83, 0.98 | |
| LkCa 15 | 159 ± 1 | B7 – J | 64.0 | 53.7 | 64 | 0.84, 1.0 | |
| Oph IRS 48 | 134 ± 2 | B9 – Q | 70.6 | 33.3 | 59.1 | 0.47, 0.84 | |
| RY Lup | 159 ± 2 | B7 – H | 71.9 | < | 15 | < 0.20 | |
| MWC758 | 160 ± 2 | B7 – Y | 80.0 | < | 15 | < 0.19 | |
| PDS 70 | 113 ± 1 | B7 – J | 81.0 | 45.0 | 54.0 | 0.56, 0.67 | |
| J1608 | 156 ± 6 | B6 – H | 81.0 | 45.0 | 49.9 | 0.56, 0.82 | |
| RXJ1604.3-2130A | 150 ± 1 | B6 – R’ | 83.0 | 54.9 | 63.7 | 0.66, 0.77 | |
| Sz 91 | 159 ± 2 | B7 – Ks | 87.5 | 46.0 | 50.9 | 0.52, 0.58 | |
| HD 34282 | 312 ± 5 | B7 – J | 133.9 | 124.2 | 132.7 | 0.93, 0.99 | |
| HD142527 | 157 ± 1 | B7 – Ks | 165, 205 | 78.5 | 157.0 | 0.38, 0.95 |
Notes. Known binary systems are indicated with the name in italic. We report the peak of the millimeter intensity beyond the cavity, along with the position of the inner radius and peak in scattered light. When the cavity is not detected down to thecoronagraph radius in scattered light, we use the symbol <. The position of the scattered light cavity (Rcav,PI), defined as the mean between Rin,PI and Rpeak,PI, is used in Fig. 10. References. HD 100546: Pinilla et al. (2018b); Garufi et al. (2016), HD 169142: Fedele et al. (2017); Pohl et al. (2017a); Bertrang et al. (2018), V4046 Sgr: Rosenfeld et al. (2013); Avenhaus et al. (2018), HD 100453: van der Plas et al. (2019); Benisty et al. (2017), T Cha: Hendler et al. (2018); Pohl et al. (2017b), UX Tau: Pinilla et al. (2018b), Menard (in prep.); HD 143006: Benisty et al. (2018); Pérez et al. (2018a), DoAr44: Casassus et al. (2018); Avenhaus et al. (2018), CQ Tau: Pinilla et al. (2018b); Benisty (in prep), J1852: This work, HD 97048: van der Plas et al. (2017b); Ginski et al. (2016), LkCa 15: Andrews et al. (2011); Thalmann et al. (2015, 2016), HD 135344B: Pinilla et al. (2018b); Stolker et al. (2016), Oph IRS 48: van der Marel et al. (2013); Bruderer et al. (2014); Geers et al. (2007), RY Lup: Pinilla et al. (2018b); Langlois et al. (2018), MWC758: Marino et al. (2015); Benisty et al. (2015), RXJ1604.3-2130A: Pinilla et al. (2018a, 2015), PDS 70: Long et al. (2018); Keppler et al. (2018), J1608:Ansdell et al. (2016), This work, Sz 91: Canovas et al. (2016); Tsukagoshi et al. (2014), HD 34282: van der Plas et al. (2017a), de Boer (in prep.), HD 142527: Boehler et al. (2017); Avenhaus et al. (2014).
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