Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/10261/2667
Title: Disks around Hot Stars in the Trifid Nebula
Keywords: Dust, extinction
ISM : HII regions
ISM : individual : Trifid
Stars : formation
Description: 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 (150-200 K) around several members of the cluster exciting the HII region, and other stars undetected at optical wavelengths. Complementary VLA observations 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 $9.7\mu m$ silicate band is seen in emission. One young stellar source shows indications of crystalline silicates in the circumstellar dust.
Peer reviewed
URI: http://dspace.mediu.edu.my:8181/xmlui/handle/10261/2667
Other Identifiers: arXiv:astro-ph/0101435v2
http://hdl.handle.net/10261/2667
Appears in Collections:Digital Csic

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