Table 1
Stellar properties of the components of DS Tuc.
Parameter | DS Tuc A | DS Tuc B | Ref. |
---|---|---|---|
α (2000) | 23:39:39.481 | 23:39:39.270 | 1 |
δ (2000) | −69:11:44.709 | −69:11:39.495 | 1 |
μα (mas yr−1) | 79.464 ± 0.074 | 78.022 ± 0.064 | 1 |
μδ (mas yr−1) | − 67.440 ± 0.045 | − 65.746 ± 0.037 | 1 |
RV (km s−1) | 8.0 ± 0.8 | 6.1 ± 0.1 | 2 |
RV (km s−1) | 7.8815 ± 0.0081 (a) | – | 3 |
RV (km s−1) | 7.20 ± 0.32 | 5.32 ± 0.65 | 1 |
RV (km s−1) | 7.4 ± 0.2 | – | 4 |
π (mas) | 22.6663 ± 0.0354 | 22.6504 ± 0.0297 | 1 |
V (mag) | 8.469 ± 0.013 | 9.84 ± 0.01 | 5 |
B − V (mag) | 0.693 ± 0.017 | 1.00 ± 0.01 | 5 |
V − I (mag) | 0.77 ± 0.01 | 1.16 ± 0.01 | 2 |
G (mag) | 8.3193 ± 0.0010 | 9.3993 ± 0.0014 | 1 |
BP-RP (mag) | 0.8908 | 1.2769 | 1 |
J2MASS (mag) | 7.122 ± 0.024 | 7.630 ± 0.058 | 6 |
H2MASS (mag) | 6.759 ± 0.023 | 7.193 ± 0.034 | 6 |
K2MASS (mag) | 6.676 ± 0.034 | 7.032 ± 0.063 | 6 |
T (mag) | 7.771 ± 0.018 | 8.607 ± 0.030 | 7 |
Spectral type | G6V | K3Ve | 2 |
Teff (K) | 5542 ± 21 | 4653 ± 18 | 5 |
Teff (K) | ![]() |
![]() |
1 |
log g | 4.60 ± 0.15 | – | 3 |
[Fe/H] (dex) | − 0.08 ± 0.06 | – | 3 |
![]() |
− 4.166 ± 0.015 | – | 3 |
![]() |
− 4.09 | – | 8 |
v sin i (km s−1) | 18.3 ± 1.8 | 14.6 ± 1.5 | 2 |
v sin i (km s−1) | 15.5 ± 1.5 | – | 3 |
Prot (d) | 2.85 ± 0.02 | – | 3 |
log LX | 30.21 (b) | 3 | |
log LX ∕Lbol | −3.35 (b) | 3 | |
EW Li (mÅ) | 216 | 232 | 2 |
Mass (M⊙) | 0.959 ± 0.031 (c) | 0.782 ± 0.022 (c) | 3 |
Radius (R⊙) | 0.872 ± 0.027 (c) | 0.769 ± 0.033 (c) | 3 |
Radius (R⊙) | ![]() |
![]() |
1 |
Age (Myr) | 40 ± 5 | 9 |
Notes. (a) Offline HARPS DRS (see Sect. 4.1). (b)A+B. (c) Derived using the PARAM web interface (da Silva et al. 2006).
References. 1. Gaia Collaboration (2018); 2. Torres et al. (2006); 3. this paper; 4. Nordström et al. (2004); 5. Pecaut & Mamajek (2013); 6. Skrutskie et al. (2006); 7. Stassun et al. (2018); 8. Henry et al. (1996); 9. Kraus et al. (2014).
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