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Fig. 4


Top: a) the binding energy for TMR-1ABC compared with other wide systems in nearby young clusters with a substellar/planetary-mass secondary. Bottom: b) total system mass as a function of separation in AU for TMR-1ABC and other low-binding energy systems (bold squares; see text for details). Included for comparison are wide (500–5000 AU) systems in Taurus (plotted as diamonds) from Kraus & Hillenbrand (2009).

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