Table 1
Fundamental parameters of lower mass main-sequence systems (Sect. 4.1) ordered by increasing mass of the primary star A.
| Name | Star | M/M⊙ | R/R⊙ | log (Teff) | log (L/L⊙) | [Fe/H] | Ref. |
|
|
|||||||
| Kepler-16 | A | 0.6897(34) | 0.6489(13) | 3.648(15) | −0.829(40) | −0.04(8) | |
| B | 0.2026(7) | 0.2262(5) | (...) | (...) | [s] | 1, 2 | |
| M55 V54 | A | 0.7259(150) | 1.0060(90) | 3.796(5) | 0.140(21) | −1.86(15) | |
| B | 0.5550(81) | 0.5280(50) | 3.701(8) | −0.799(33) | [c] | 3, 4 | |
| V565 Lyr * | A | 0.9956(33) | 1.1011(68) | 3.748(7) | 0.029(12) | 0.31(6) | |
| B | 0.9293(32) | 0.9708(89) | 3.735(10) | −0.134(18) | [s] | 5 | |
| V636 Cen | A | 1.0518(48) | 1.0186(43) | 3.771(6) | 0.053(25) | −0.20(8) | |
| B | 0.8545(30) | 0.8300(43) | 3.699(9) | −0.413(35) | [s] | 6 | |
| V568 Lyr * | A | 1.0886(31) | 1.4203(58) | 3.752(7) | 0.266(35) | 0.26(6) | |
| B | 0.8292(26) | 0.7997(15) | 3.675(7) | −0.535(27) | [s] | 5, 7 | |
Notes. The final digits, in parentheses, give the 1σ errors. The determination method of [Fe/H] is indicated in the [Fe/H] column (for details see text). Models marked by an asterisk in the first column were computed with a different set of opacities (for more details, see Sect. 2).
Reference. (1) Doyle et al. (2011); (2) Winn et al. (2011); (3) Kaluzny et al. (2014); (4) Harris (1996); (5) Brogaard et al. (2011); (6) Clausen et al. (2009); (7) Yakut et al. (2015).
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