Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-06-04
Astronomy and Astrophysics
Astrophysics
4 pages, accepted for publication in Astronomy & Astrophysics Letters
Scientific paper
Massive, large scale star counts in the J band provided by the Deep Near Infrared Survey of the Southern Sky (DENIS) are used for the first time to draw out an extinction map of the Chamaeleon I dark cloud. We derived a 2 arcminutes resolution map of the cloud from J star counts within an area of 1.5 x 3 degres around the centre of the cloud using an adaptive grid method and applying a wavelet decomposition. A comparison of our extinction map with the cold contribution of the IRAS 100 microns emission shows an almost perfect matching. It is shown that J star counts supersede optical counts on Schmidt plate where Av > 4.
Batz Bertrand de
Bertre Th. Le
Cambresy Laurent
Copet E.
Epchtein Nicolas
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