Fig. 5

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Schematic configurations of multiple stellar systems with exoplanets. Orange circles are main-sequence stars, cyan circles are subgiant and giant stars, white circles are white dwarfs, small brown circles are brown dwarfs, and black dots are planets. We display our 212 systems with grey background, except for the two systems with circumbinary planets, namely RR Cae and Kepler-16, with green background, and the three systems from Table 4 with planets around both stars, with white background. The systems are sorted by increasing separation from the planet host star to the closest companion star. The abscissa is in logarithmic scale. We also display the Solar System in yellow as a comparison.
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