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Distributions of Wide Binary Stars in Theory and in Gaia Data. II. Reconstruction of Sample Probability Density of True Orbit Sizes

  • Authors: Valeri V. Makarov

Valeri V. Makarov 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 5.

The differential function Φ(l) (Equation (7)) related to the power index γ(l) in the tail of PDF(a) reconstructed by the IF technique. The dashed red line shows the same linear fit for the interval l ∈ [3, 5] as in Figure 3, for reference.

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