Fig. 15
Log (L∕L⊙) vs. age diagram for USco1621 B (purple circle) and USco1556 B (red triangle), together with Ames-COND model isomasses from Allard et al. (2001) and Baraffe et al. (2003). Theoretical hydrogen- and deuterium-burning mass limits are marked in dark grey. Other known young wide substellar companions with separations above 1000 AU from Kirkpatrick et al. (2001); Bouy et al. (2003); Allers et al. (2010); Goldman et al. (2010); Todorov et al. (2010); Kuzuhara et al. (2011); Aller et al. (2013); Dupuy et al. (2014); Naud et al. (2014); Bowler & Hillenbrand (2015) (green diamonds) are also included.
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