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

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Fig. 13.

Relative differences of parameters derived for δ Ori for eight seasons (Table B.3). In all models, the effective temperature T₁ of the primary (Aa1) and the third light l₃ were fixed. Season 2016 was taken as a reference. Explanations of the parameters can be found in Table 9.

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