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Fig. 12

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Binary fraction in 47 Tuc as a function of (projected) distance from the cluster center, in units of half light radii Rhl. The observed discovery fraction is shown in radial bins of 1000 stars (dark blue), with error bars representing uncertainties, calculated by varying the binary probability threshold 0.4 < P(χ2) < 0.6 and adding statistical noise in quadrature. The predicted binary fraction from the CMC simulation is shown as the orange dotted line. The grey dashed line represents a fitted power law, fbin(R/Rhl)β${f_{{\rm{bin}}}} \propto {\left( {R{/_{{R_{hl}}}}} \right)^\beta }$, with β = (−0.2 ± 0.07); shaded areas show the uncertainty intervals.

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