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Table 5.

Best-fitting final parameters of model atmospheres matching the observed spectra.

AL Ari

Grid best model
Best fit parameters
Parameter Primary Secondary Primary Secondary Unit
[M/H] −0.4 −0.6 −0.42 ± 0.07 −0.60 ± 0.13 dex
Teff 6600 5600 6578 ± 82 5560 ± 192 K
log g( * ) 4.2 4.5 4.30 ± 0.15 4.26 ± 0.37 dex
ξ 1.5 2.0 1.54 ± 0.14 2.00 ± 0.46 km s−1
ζ( ⋆ ) 5.8 2.6 km s−1
Vrot sin i 17 13 17.11 ± 0.61 12.65 ± 1.50 km s−1
Reduced χ2 8.304440
8.349265

AL Dor

Grid best model
Best fit parameters
Parameter Primary Secondary Primary Secondary Unit

[M/H] −0.1 −0.1 −0.11 ± 0.05 −0.11 ± 0.05 dex
Teff 6100 6100 6076 ± 70 6051 ± 70 K
log g( * ) 4.4 4.4 4.38 ± 0.18 4.38 ± 0.17 dex
ξ 1.4 1.3 1.36 ± 0.18 1.29 ± 0.17 km s−1
ζ( ⋆ ) 3.1 3.4 3.1 ± 0.5 3.4 ± 0.5 km s−1
Vrot sin i 4 4 4.08 ± 0.60 3.90 ± 0.66 km s−1
Reduced χ2 16.507021
16.596123

FM Leo

Grid best model
Best fit parameters
Parameter Primary Secondary Primary Secondary Unit

[M/H] −0.1 −0.1 −0.10 ± 0.06 −0.10 ± 0.06 dex
Teff 6400 6400 6425 ± 88 6418 ± 96 K
log g( * ) 4.1 4.2 4.11 ± 0.17 4.18 ± 0.19 dex
ξ 1.6 1.5 1.61 ± 0.15 1.49 ± 0.17 km s−1
ζ( ⋆ ) 5.8 4.3 km s−1
Vrot sin i 11 11 11.0 ± 0.6 11.0 ± 0.6 km s−1
Reduced χ2 17.056393
17.148460

BN Scl

Grid best model
Best fit parameters
Parameter Primary Secondary Primary Secondary Unit

[M/H] −0.2 −0.3 −0.18 ± 0.08 −0.24 ± 0.10 dex
Teff 6300 6300 6304 ± 93 6296 ± 148 K
log g( * ) 4.0 4.3 4.15 ± 0.18 4.37 ± 0.30 dex
ξ 1.6 1.7 1.62 ± 0.17 1.69 ± 0.30 km s−1
ζ( ⋆ ) 5 5 km s−1
Vrot sin i 24 19 23.55 ± 1.04 18.73 ± 1.43 km s−1
Reduced χ2 13.856710
13.931628

Notes. The simultaneous solution obtained with the GSSP_binary module for each eclipsing binary using the disentangled spectra of both components. ( * )Fixed on the values available in the grid of atmosphere models that are the closest to the values originated from the dynamical solution. ( ⋆ )Fixed on the values resulting from solutions with the use of GSSP_single module.

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