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).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.