Open Access
Table D.1
Rotation periods, v sin i, corotation radii, magnetic truncation radii for a magnetic field of 1 kG, and sublimation radii as computed from Eq. (2) with Tsub = 1500 K for oursample. The last column gives the references for the rotational period or the v sin i.
| Target name | v sin i [km/s] | Prot [days] | Rco [au] | Rmag [au] | Rsub [au] | References |
|---|---|---|---|---|---|---|
| DG Tau | 6.3 | 0.06 | 0.016 | 0.05 – 0.10 | Bouvier et al. (1993) | |
| DR Tau | 5.0 | 0.07 | 0.045 | 0.07 – 0.14 | Percy et al. (2010) | |
| RY Tau | 5.6 | 0.09 | 0.114 | 0.15 – 0.37 | Herbst et al. (1987) | |
| T Tau N | 2.8 | 0.06 | 0.060 | 0.11 – 0.26 | Herbst (1986) | |
| GQ Lup | 8.4 | 0.07 | 0.044 | 0.04 – 0.08 | Donati et al. (2012) | |
| IM Lup | 7.2 | 0.06 | 0.12 | 0.05 – 0.11 | from TESS (unpublished) | |
| RU Lup | 3.7 | 0.04 | 0.032 | 0.05 – 0.10 | Covino et al. (1989) | |
| RY Lup | 3.9 | 0.06 | 0.036 | 0.06 – 0.14 | Bouvier et al. (1986) | |
| S CrA N | 3.6 | 0.04 | 0.047 | 0.06 – 0.11 | Nowacki et al. (private comm.) | |
| S CrA S | 12 | 3 | 0.04 | 0.028 | 0.04 – 0.07 | Sullivan et al. (2019) |
| VV CrA SW | 3.6 | 11 | 0.09 | 0.046 | 0.04 – 0.08 | Sullivan et al. (2019) |
| V2062 Oph | 2.96 | 0.05 | 0.030 | 0.04 – 0.10 | Bouvier et al. (2020a) | |
| V2129 Oph | 6.53 | 0.07 | 0.094 | 0.06 – 0.13 | Alencar et al. (2012) | |
| AS 205 N | 2.7/6.78 | 0.04/0.07 | 0.012 | 0.08 – 0.20 | Covino et al. (1992)/Artemenko et al. (2010) | |
| AS 353 | 10 | 7 | 0.1 | 0.044 | 0.05 – 0.10 | Rei et al. (2018) |
| DI Cha | 30 | 1.5 | 0.04 | 0.056 | 0.14 – 0.40 | Bouvier et al. (1986) |
| TW Hya | 3.56 | 0.05 | 0.023 | 0.02 – 0.04 | Donati et al. (2011) |
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