Table 1
Stellar properties and observational details of the sample of compact discs studied in this work.
| Source | M* (M⊙) |
L* (L⊙) |
Dist. (pc) |
vhel (km s−1) |
Inclination (°) |
Rin (au) |
Rdust,95% (au) |
Obs. date dd/mm/yyyy |
Int. time (min) |
References M*/L*/vhel/i/Rdust |
|---|---|---|---|---|---|---|---|---|---|---|
| BP Tau | 0.52 | 0.40 | 129 | 16.76 | 23.6 | 0.04 | 41 | 20/02/2023 | 29.0 | m1, l1, v1, i1, d1 |
| CX Tau | 0.37 | 0.26 | 128 | 19.30 | 55.1 | 0.04 | 38 | 20/02/2023 | 60.0 | m2, l2, v2, i2, d2 |
| CY Tau | 0.31 | 0.26 | 128 | 15.10 | 32.0 | 0.04 | <64 | 20/02/2023 | 60.0 | m2, l2, v2, i3, d3 |
| DN Tau | 0.52 | 0.70 | 128 | 18.80 | 35.2 | 0.06 | 61 | 28/09/2023 | 60.0 | m1, l1,v2, i4, d1 |
| DR Tau | 0.93 | 0.63 | 195 | 27.60 | 5.4 | 0.06 | 54 | 04/03/2023 | 27.8 | m1, l1,v3, i4, d1 |
| FT Tau | 0.34 | 0.15 | 127 | 17.24 | 35.5 | 0.03 | 45 | 20/02/2023 | 30.0 | m1, l1, v4, i4, d1 |
| RNO 90 | 1.50 | 2.14 | 117 | −10.10 | 37.0 | 0.10 | <47 | 25/08/2023 | 33.4 | m3, l3, v5, i5, d3 |
| XX Cha | 0.36 | 0.29 | 190 | 16.26 | 39.7 | 0.04 | <25 | 31/08/2023 | 60.0 | m4, l4, v6, i6, d3 |
Notes. All distances have been acquired from GAIA (Gaia Collaboration 2018). References (mass, luminosity, heliocentric velocity, inclination, dust radii): m1 – Long et al. (2019), m2 – Simon et al. (2017), m3 – Banzatti et al. (2022), m4 – Manara et al. (2016), l1 – Long et al. (2019), l2 – Herczeg & Hillenbrand (2014), l3 – Banzatti et al. (2022), l4 – Manara et al. (2016), v1 – Fang et al. (2018), v2 – Banzatti et al. (2019), v3 – Ardila et al. (2002), v4 – Roccatagliata et al. (2020), v5 – Banzatti et al. (2022), v6 – Nguyen et al. (2012), i1 – Gasman et al. (2025), i2 – Facchini et al. (2017), i3 – Simon et al. (2017), i4 – Long et al. (2019), i5 – Bosman & Bergin (2021), i6 – this work, d1 – Long et al. (2019), d2 – Facchini et al. (2019), d3 – estimated in this work.
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