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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 3.

Left: the differential function Φ(l) (Equation (7)) related to the power index γ(l) in the tail of PDF(a) reconstructed by the direct mapping technique. The dashed red line shows the linear fit for the interval l ∈ [3, 5]. Right: the empirical function Φ(λ) estimated from the actual histogram of ﹩\lambda ={{\mathrm{log}}}_{10}\,(s)﹩. The dashed red line is the same linear fit as in the left panel, for reference.

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