Table A.4
Projected rotational velocity (v sin i) derived by the previous study, period measured from TESS light curves, stellar age, mass, convective turnover time (τc), and Rossby number (NR) of the 64 PMS stars.
| Object Name | v sin i | Period | Age | Mass | τc | log NR |
|---|---|---|---|---|---|---|
| [km • s−1] | [d] | [Myr] | [M⊙] | [d] | ||
| Taurus molecular cloud | ||||||
| AA Tau | 12.7 | 7.03 | 7.9 | 0.53 | 75 | -1.03 |
| BP Tau | 11.4 | 7.18 | 6.5 | 0.53 | 252 | -1.55 |
| CQ Tau | 107.5 | 12.16 | 7.3 | 1.19 | 22 | -0.26 |
| DE Tau | 10.0 | 5.69 | 6.2 | 0.39 | 232 | -1.61 |
| DF Tau | 19.1 | 10.63 | 5.7 | 0.34 | 225 | -1.33 |
| DG Tau | 21.7 | 17.99 | 7.2 | 0.82 | 102 | -0.75 |
| DK Tau | 11.4 | 6.56 | 6.9 | 0.78 | 161 | -1.39 |
| DM Tau | 10.0 | 7.32 | 6.9 | 0.35 | 240 | -1.52 |
| DN Tau | 9.4 | 6.49 | 6.1 | 0.44 | 234 | -1.56 |
| DR Tau | 10.0 | 16.47 | 7.7 | 0.81 | 31 | -0.28 |
| FP Tau | 23.5 | 2.18 | 6.5 | 0.34 | 232 | -2.03 |
| GM Aur | 13.0 | 5.43 | 6.9 | 0.87 | 143 | -1.42 |
| HBC 407 | 10.0 | 3.45 | 7.8 | 0.76 | 35 | -1.00 |
| HP Tau | 66.0 | 0.44* | 7.3 | 0.94 | 57 | -1.88 |
| IQ Tau | 12.0 | 6.63 | 7.2 | 0.58 | 172 | -1.41 |
| LkCa 04 (24 Nov) | 26.1 | 3.37 | 6.5 | 0.48 | 244 | -1.86 |
| LkCa 04 (26 Nov) | 26.1 | 3.37 | 6.5 | 0.48 | 244 | -1.86 |
| LkCa 15 (27 Feb) | 12.5 | 5.13 | 7.6 | 0.76 | 51 | -0.99 |
| LkCa 15 (6 Mar) | 12.5 | 5.13 | 7.0 | 1.04 | 86 | -1.22 |
| RY Tau | 50.8 | 5.24 | 6.6 | 1.83 | 63 | -1.08 |
| T Tau | 21.0 | 14.96 | 6.6 | 1.79 | 69 | -0.66 |
| UX Tau | 20.7 | 6.42 | 7.1 | 1.22 | 63 | -0.99 |
| V1354 Tau | 1.46 | 7.5 | 0.94 | 32 | -1.34 | |
| ρ Ophiuchi molecular cloud | ||||||
| V2062 Oph | 8.5 | 5.79* | 6.1 | 0.90 | 266 | -1.33 |
| V2129 Oph | 15.8 | 5.11* | 6.1 | 0.52 | 240 | -1.67 |
| V2247 Oph | 43.1 | 1.11* | 6.4 | 0.40 | 236 | -2.25 |
| Lupus star-forming region | ||||||
| GQ Lup | 10.77 | 6.2 | 0.78 | 261 | -1.38 | |
| Chamaeleon I star-forming region | ||||||
| CHX22 | 11.3 | 7.37* | 6.6 | 1.87 | 62 | -0.77 |
| CR Cha | 36.7 | 2.21* | 6.8 | 1.56 | 57 | -1.35 |
| CV Cha | 30.3 | 3.00* | 6.6 | 1.53 | 93 | -1.47 |
| CW Cha | 29.6 | 1.06* | 7.8 | 0.43 | 117 | -2.20 |
| Orionis OB 1c association | ||||||
| CO Ori | 56.6 | 2.32* | 6.3 | 2.55 | 34 | -0.99 |
| COUP 1287 | 32.7 | 0.78* | 7.4 | 0.36 | 226 | -2.44 |
| COUP 1423 | 40.7 | 1.62* | 6.0 | 0.29 | 225 | -2.11 |
| GW Ori | 41.7 | 5.67* | 5.8 | 3.56 | 31 | -0.59 |
| HBC 167 | 18.0 | 7.52* | 6.7 | 1.91 | 74 | -0.99 |
| OV Ori | 20.1 | 2.31* | 6.9 | 0.88 | 133 | -1.67 |
| V1044 Ori | 22.3 | 4.66* | 6.5 | 2.23 | 31 | -0.65 |
| V1458 Ori | 20.3 | 11.31* | 4.3 | 0.36 | 217 | -1.24 |
| Upper Scorpius association | ||||||
| 2MASS J16123916-1859284 | 12.3 | 3.00* | 7.0 | 0.49 | 248 | -1.87 |
| V1149 Sco | 7.1 | 1.40 | 36 | |||
| AB Doradus moving group | ||||||
| HIP 17695 | 3.86 | 7.7 | 0.26 | 252 | -1.82 | |
| β Picoris moving group | ||||||
| AU Mic | 8.0 | 4.80 | 7.7 | 0.51 | 99 | -1.31 |
| “Cha-Near” region | ||||||
| RX J1147.7-7842 | 6.6 | 0.30 | 229 | |||
| RX J1204.6-7731 | 9.5 | 4.79 | 6.6 | 0.25 | 225 | -1.67 |
| η Chamaeleontis cluster | ||||||
| RECX 04 | 6.97 | 7.0 | 0.50 | 245 | -1.55 | |
| RECX 06 | 1.84 | 6.9 | 0.25 | 227 | -2.09 | |
| RECX 07 | 30.0 | 1.99* | 6.8 | 0.88 | 155 | -1.88 |
| RECX 09 | 1.94 | 6.0 | 0.08 | 186 | -1.98 | |
| RECX 10 | 11.0 | 8.74 | 7.3 | 0.68 | 108 | -1.09 |
| RECX 11 | 4.98 | 7.4 | 0.87 | 62 | -1.09 | |
| RECX 15 | 30.0 | 0.98* | 7.0 | 0.21 | 222 | -2.39 |
| TW Hydrae association | ||||||
| TWA 1 | 15.0 | 7.08 | 7.2 | 0.67 | 138 | -1.29 |
| TWA 5B | 59.0 | 0.73 | 6.2 | 0.25 | 224 | -2.49 |
| TWA 6 | 0.54 | 7.3 | 0.73 | 97 | -2.25 | |
| TWA 7 | 63.2 | 4.92 | 6.8 | 0.25 | 227 | -1.66 |
| TWA 8A | 5.0 | 4.63 | 6.8 | 0.25 | 226 | -1.69 |
| TWA 8B | 5.0 | 4.73 | 7.1 | 0.07 | 180 | -1.58 |
| TWA 9A | 5.03 | 6.7 | 0.55 | 266 | -1.72 | |
| TWA 9B | 4.96 | 7.0 | 0.21 | 222 | -1.65 | |
| TWA 14 | 0.63 | 7.0 | 0.49 | 252 | -2.60 | |
| TWA 22 | 0.73 | 7.0 | 0.07 | 179 | -2.39 | |
| TWA 25 | 12.9 | 5.05 | 7.0 | 0.59 | 192 | -1.58 |
v sin i; the projected rotational velocity from the Catalog of Stellar Rotational Velocities (Glebocki & Gnacinski 2005). (*) The rotational periods are estimated with their v sin i because TESS light curve were not obtained.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.