Disks around hot stars in the Trifid nebula

We report on mid-IR observations of the central region in the Trifid nebula , carried out with ISOCAM in several broad-band infrared filters and in the low resolution spectroscopic mode provided by the circular variable filter . Analysis of the emission indicates the presence of a hot dust component ( 500 to 1000 K) and a warm dust component at lower temperatures (similar to 150-200 K) around several members of the cluster exciting the I-III region, and other stars undetected at optical wavelengths. Complementary VLA obser vations suggest that the mid-IR emission could arise from a dust cocoon or a circumstellar disk, evaporated under the ionization of the central source and the exciting star of the nebula. In several sources the 9.7 mum silica te band is seen in emission. One young stellar source shows indications of crystalline silicates in the circumstellar dust.