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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 1.

Monte Carlo-simulated histograms of f, which is the fractional projection factor given by Equation (3), for three cases of power-law eccentricity distributions, ﹩{\alpha }^{{\prime} }=-1﹩ (left), ﹩{\alpha }^{{\prime} }=+0.15﹩ (center), and ﹩{\alpha }^{{\prime} }=+1﹩ (right).

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