Low mass T Tauri and young brown dwarf candidates in the Chamaeleon II dark cloud found by DENIS

We define a sample designed to select low-mass T Tauri stars and young brow n dwarfs using DENIS data in the Chamaeleon II molecular cloud. We use a st ar count method to construct an extinction map of the Chamaeleon II cloud. We select our low-mass T Tauri star and young brown dwarf candidates by the ir strong infrared color excess in the I - J/J - K-s color-color dereddened diagram. We retain only objects with colors I - J greater than or equal to 2, and spatially distributed in groups around the cloud cores. This provid es a sample of 70 stars of which 4 are previously known T Tauri stars. We h ave carefully checked the reliability of all these objects by visual inspec tion of the DENIS images. Thanks to the association of the optical I band t o the infra-red J and K-s bands in DENIS, we can apply this selection metho d to all star formation regions observed in the southern hemisphere. We als o identify six DENIS sources with X-ray sources detected by ROSAT. Assuming that they are reliable low-mass candidates and using the evolutionary mode ls for low-mass stars, we estimate the age of these sources between 1 Myr a nd <10 Myr.