Results of the best fit of the OSTAR grid of synthetic spectra to the observed ones.
|Quantity||Component A||Component Ba|
|Teff (K)||32 506 ± 23||32 544 ± 48|
|log (g[cgs])||3.738 ± 0.014||3.706 ± 0.009|
|vsini (km s-1)||200.4 ± 2.9||61.41 ± 0.47|
|L R||0.5712 ± 0.0021||0.4288 ± 0.0021|
|RV (km s-1)||−20.2 ± 2.6||−19.72 ± 0.36|
Notes. The optimised parameters are: the effective temperature Teff, gravitational acceleration g, projected rotational velocity vRsini, fractional luminosity LR, RV, and metallicity Z.
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