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Table 7

Mdwarfs in wide physical binaries with FGK-type primaries in common with the CARMENES GTO survey.

Primary Secondary

Name SpT [Fe/H] [dex] Name Karmn SpT Teff [K] logg [dex] [Fe/H]corr [dex]
V538 Aur K1 V 0.04 ± 0.02 HD 233153 J05415+534 M1.0 V 3825 ± 14 4.94 ± 0.10 − 0.02 ± 0.06
V869 Mon K0/2 V − 0.11 ± 0.03 GJ 282 C J07361−031 M1.0 V 3825 ± 12 5.06 ± 0.08 − 0.04 ± 0.06
HD 154363 K5 V − 0.62 ± 0.05 HD 154363 B J17052−050 M1.5 V 3587 ± 14 4.89 ± 0.10 − 0.39 ± 0.07
θ Boo A F7 V − 0.09 ± 0.01 θ Boo B J14251+518 M2.5 V 3551 ± 22 4.90 ± 0.10 − 0.14 ± 0.06
HD 16160 K3 V − 0.20 ± 0.02 BX Cet J02362+068 M4.0 V 3335 ± 45 4.91 ± 0.10 − 0.24 ± 0.12
o02 Eri A K0.5 V − 0.37 ± 0.02 o02 Eri C J04153−076 M4.5 V 3179 ± 61 5.00 ± 0.18 − 0.30 ± 0.17
ρ Cnc G8 V 0.29 ± 0.04 ρ Cnc B J08526+283 M4.5 V 3321 ± 37 4.87 ± 0.08 − 0.10 ± 0.11

Notes. Metallicities of the FGK-type primary stars from Montes et al. (2018), except for θ Boo A, which is from Tabernero et al. (2021). Stellar atmospheric parameters of the M-dwarf secondaries (Teff, log g, and [Fe/H]) as computed in this work.

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