Spatial distribution of the spectroscopically confirmed members of C69. Active accretors according to the saturation criterion are highlighted in red. Information regarding infrared excess (as a proxy for the presence of disk, from Barrado y Navascués et al. 2007) is provided by surrounding those sources with larger circumferences. The more massive population of C69 (λ Ori itself and the B stars) is shown with gray four-pointed stars. Finally, the members with X-ray detections are shown with five-pointed blue stars.