The PAIRS project: a global formation model for planets in binaries - II. Gravitational perturbation effects from secondary stars

Open Access

Fig. C.3

Circumsecondary in situ formation: Initial planetary position relative to the disk truncation radius, a_p,0/R_trunc or $a_{p, 0} / R_{trunc}^{'}$ $Mathematical equation: $\[a_{\mathrm{p}, 0} / R_{\text {trunc}}^{\prime}\]$$ , versus final planet mass. The color bar shows the binary periastron distance. Circle markers represent stable planets from circumsecondary simulations presented in this section, while green crosses represent stable planets from set A simulations.

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