Spectrum of the secondary component and new orbital elements of the massive triple star δ Ori A

Open Access

Fig. 7.

Pseudo-χ² in Fourier space vs. mass ratio q₁ = m₂/m₁. This is related to the two-step disentangling method, to its second step, when the signal of the secondary component (Aa2) was sought for in the residuals.

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