Table C.1.
Stellar observational data used in Fig. 9 and Fig. 10. The respective uncertainties are given when available. Missing data is represented by "—".
Name | Age [Myr] | M⋆ [M⊙] | R⋆ [R⊙] | P⋆ [d] | BI [G] | BV [G] | BQU [G] |
---|---|---|---|---|---|---|---|
AU Mic | 23 ± 11 | 0.50 ± 0.032 | 0.75 ± 0.032 | 4.86 ± 0.012 | 2310 ± 2001 | 881 | 2000 ± 2001 |
WW Psa | 27 ± 73 | 0.19 ± 0.043 | 0.70 ± 0.133 | 2.37 ± 0.013 | 2750 ± 2503 | — | — |
TX Psa | 27 ± 73 | 0.11 ± 0.033 | 0.52 ± 0.103 | 1.09 ± 0.013 | 2750 ± 2503 | — | — |
V1124 Oria | 1.24 | 0.264 | 2.154 | 8.184 | 2090 ± 3404 | — | — |
V1123 Oria | 0.84 | 0.354 | 2.594 | 7.644 | 2510 ± 4104 | — | — |
V1568 Oria | 1.34 | 0.404 | 2.374 | 5.544 | 1420 ± 2304 | — | — |
Upp Sco 55b | 55 | 0.105 | 0.525 | 2.90 ± 0.305 | 2300 ± 13005 | — | — |
TWA 9B | 106 | 0.306 | 0.916 | 3.986 | 3100 ± 2006 | — | — |
TWA 8A | 11 ± 57 | 0.45 ± 0.107 | 0.80 ± 0.207 | 4.58 ± 0.017 | 6000 ± 5007 | 7207 | — |
GJ 490B | 35-3508 | 0.339 | 0.349 | 0.549 | 3200 ± 4009 | 6809 | — |
V2247 Opha | 1.010 | 0.3510 | 2.0010 | 3.4010 | 2700 ± 10011 | 9010 | — |
TWA 7 | 17 ± 1012 | 0.62 ± 0.0312 | 0.80 ± 0.1012 | 5.00 ± 0.0112 | 2700 ± 20011 | 5012 | — |
Notes. aDespite the young age of those stars, they are identified as NTTS or weak accretors and thus, included in the list. bP⋆ calculated from vsini data.
References. (1) Kochukhov & Reiners (2020); (2) Plavchan et al. (2020); (3) Messina et al. (2017); (4) Yang & Johns-Krull (2011); (5) Reiners et al. (2009); (6) Yang et al. (2008); (7) Hill et al. (2019); (8) Klutsch et al. (2014); (9) Phan-Bao et al. (2009); (10) Donati et al. (2010); (11) Lavail et al. (2019), (12) Nicholson et al. (2021).
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