Table 1
Stellar parameters.
Name | Other name | Sp type | Ref | d | T eff | L ∗ |
|
||||||
(pc) | (K) | (L⊙) | ||||
|
||||||
TWA 01 | TW Hya | M2.5 | 1 | 56 | 3400 | 0.23 |
TWA 02 | CD-29 8887 | M2 | 2 | 52 | 3700 | 0.30 |
TWA 03A | Hen 3-600 | M3 | 2 | 42 | 3000 | 0.18 |
TWA 04B | HD 98800B | M5 | 3 | 47 | 4000 | 0.56 |
TWA 05A | CD-33 7795 | M3 | 3 | 50 | 3100 | 0.28 |
TWA 07 | CE Ant | M1 | 4 | 38 | 3300 | 0.15 |
TWA 10 | V1252 Cen | M2.5 | 4 | 57 | 3400 | 0.10 |
TWA 11A | HR 4796A | A0 | 5 | 67 | 10 000 | 21.3 |
TWA 12 | V1217 Cen | M2 | 6 | 32 | 3400 | 0.03 |
TWA 13A | V547 Hya A | M2 | 6 | 38 | 3700 | 0.10 |
TWA 16 | – | M1.5 | 7 | 66 | 3900 | 0.17 |
TWA 21 | HD 298936 | K3 | 8 | 69 | 4600 | 0.72 |
TWA 23 | – | M1 | 9 | 37 | 3400 | 0.07 |
TWA 25 | V1249 Cen | M0 | 9 | 44 | 3800 | 0.15 |
Notes.All distances are from Zuckerman & Song (2004). Teff and L∗ for each target were computed using VOSA (Bayo et al. 2008). References for spectral type (Sp Type) are: (1) Vacca & Sandell (2011); (2) de la Reza et al. (1989); (3) Gregorio-Hetem et al. (1992); (4) Webb et al. (1999); (5) Houk & Fuentes-Williams (1982); (6) Sterzik et al. (1999); (7) Zuckerman et al. (2001); (8) Zuckerman & Song (2004); (9) Weinberger et al. (2004).
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