Fig. 3
Accretion in Cha II members. Plus symbols depict objects that might have Hα emission coming only from purely chromospheric emission, while black dots are objects with Hα in agreement with ongoing accretion. The solid line shows the saturation criterion by Barrado y Navascués & Martín (2003). Red circles surrounding black dots denote objects with [OI] emission at 63.18 μm detected by PACS.
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