Table 1
Stellar and disk properties of the target stars.
| Target | Age (Myr) | M* (M⊙) | T(K) | L* (L⊙) | d (pc)(a) | PA (°) | i (°) | Structures | Companions |
|---|---|---|---|---|---|---|---|---|---|
| detected | |||||||||
| HD 100546(b) | 5 | 2.5 | 10 600 | 30 | 108.1 | 140 | 46 | Gap, spiral arms | 3 |
| HD 163296(c) | 6 | 2.5 | 9000 | 34.7 | 101.0 | 137 | 43 | Rings | 3 |
| HD 169142(d) | 4–16 | 1.8 | 7800 | 9.8 | 114.9 | 5 | 13 | Rings | 3 |
| TW Hydra(e) | 3–15 | 0.8 | 4000 | 0.2 | 60.1 | 150 | 7 | Rings | 1 |
| HD 100453(f) | 11 | 1.5 | – | 6 | 103.8 | 145 | 35 | Gap, spiral arms | M dwarf |
| HD 36112(g) | 4 | 2.0 | 8200 | 22 | 155.9 | 62 | 21 | Cavity, rings, clumps, spirals | 2 |
Notes. Stellar masses, luminosities,and temperatures, where possible, have been taken from the DIANA models of the targets, which are fit to multiple data sets.
References. (a) Gaia Collaboration (2021). (b) Wichittanakom et al. (2020); Miley et al. (2019); Casassus & Pérez (2019); Jamialahmadi et al. (2018); Mendigutía et al. (2017); Pineda et al. (2014); Avenhaus et al. (2014); Walsh et al. (2014); Leinert et al. (2004). (c) Garufi et al. (2014); Wichittanakom et al. (2020). (d)Pérez et al. (2019); Panić et al. (2008); Raman et al. (2006); van Boekel et al. (2005). (e) Nayakshin et al. (2020); Sokal et al. (2018). (f)Wichittanakom et al. (2020); Rosotti et al. (2020); Yu et al. (2019); Long et al. (2017); Benisty et al. (2017); Wagner et al. (2015). (g) Isella et al. (2010); Meeus et al. (2012).
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