Configuration of the ξ Tau system constrained by multi-technique observations

Open Access

Fig. 8.

Same as Fig. 7 but the parameters of all orbits were free. The solutions differ from Fig. 7 partly because of perturbations by component C. The solutions with low Δt₁ ∼ 100 s exhibit a poor fit of eclipse duration (ECL), so the solution with high Δt₁ (and zero C_20, 1) is still preferred.

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