Fig. 8
Probability distribution function (PDF) of planets in star clusters (red, green, and cyan crosses are results of models w3-hd, w3-ld, and embedded, respectively. The blue line shows the PDF obtained from observed planets between 0.03 and 3 AU (see Eq. (12)). The red dashed line indicates a power-law distribution following
, which is obtained from a fitting to model w3-hd for 10–100 AU.
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