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Paper: The stellar population in Chamaeleon I Dark Cloud
Volume: 132, Star Formation with the Infrared Space Observatory (ISO)
Page: 158
Authors: Persi, P.; Olofsson, G.; Kaas, A. A.; Nordh, L.; Bontemps, S.; Huldtgren, M.; Andre, Ph.; Cesarsky, C. J.; Montmerle, T.; Abergel, A.; Boulanger, F.; Cesarsky, D.; Lagache, G.; Puget, J. L.; Blommaert, J.; Burgdorf, M.; Prusti, T.; Copet, E.; Davies, J.; Falgarone, E.; Perault, M.; Sibille, F.; Roth, M.
Abstract: We discuss the properties of the stellar population in a region of 0.55 sq deg of the Chamaeleon I dark cloud, combining the ISOCAM observations at 6.75 and 15 microns and the data at I, J and K_s, obtained with the Deep Near-IR Southern Sky Survey (DENIS).
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