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Table 4

Parameters of FGK-type primary stars with an M dwarf secondary.

Primary Teff/K log g/cm s−2 [Fe/H] Sp. type Ref. Secondary
HD 24421 6108 ± 26 4.30 ± 0.05 –0.32 ± 0.02 F5V 1 LSPMJ0355+5214
GJ297.2A 6414 ± 51 4.65 ± 0.09 –0.01 ± 0.03 F6.5V 2 GJ297.2B
GJ324A 5299 ± 58 4.35 ± 0.13 0.29 ± 0.04 K0IV-V 3 GJ324B
GJ3194 5644 ± 21 4.36 ± 0.05 –0.30 ± 0.02 G1.5V 3 GJ3195
BD+00549 5319 ± 46 4.48 ± 0.12 –0.88 ± 0.04 G5 4 BD+00549B
BD-064756 4494 ± 44 4.69 ± 0.06 –0.01 ± 0.03 K5-V 2 BD-064756B
HD 122972 5523 ± 22 4.36 ± 0.07 –0.01 ± 0.02 G6V 5 Ross799
GJ777A 5578 ± 22 4.27 ± 0.05 0.21 ± 0.02 G7IV-V 2 GJ777B
GJ211 5292 ± 32 4.38 ± 0.09 0.04 ± 0.02 K0V 3 GJ212
LSPMJ1204+1728N 5282 ± 34 4.41 ± 0.09 –0.18 ± 0.02 G9V 6 LSPMJ1204+1728S

Notes. All parameters for the primary components in the table were obtained from Montes et al. (2018) except for BD-06 4756 for which Mann et al. (2013) was used. The parameters for the K-type primaries with APOGEE spectra that were analysed by the SAPP (GJ 105A, GJ 338A) are given in Table 2. Column ‘Ref.’ gives the reference for the spectral type. Gray et al. (2006) used the system of Keenan & McNeil (1989) for the spectral types. References: (1) Cannon & Pickering (1993); (2) Gray et al. (2006); (3) Gray et al. (2003); (4) Lee (1984); (5) Houk & Swift (1999); (6) Grieves et al. (2018).

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