1998/09/07 by L. Cambresy, Cambresy, L.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9809073
4 pages, 3 figures, To Appear in the proceedings of the conference "Astrophysics With Infrared Surveys: A Prelude to SIRTF"
arxiv created 1998/09/07 · arxiv updated 2009/12/01
I present new results on the extinction and on the YSO content of the Chamaeleon I cloud using the star count method that I have implemented and applied to DENIS and optical data. Application of this method to other nearby Large Molecular Clouds is in progress and is briefly outlined.