Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/10261/2667
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dc.creatorLefloch, Bertrand-
dc.creatorCernicharo, José-
dc.creatorCesarsky, D.-
dc.creatorDemyk, K.-
dc.creatorMiville-Deschenes, M.A.-
dc.creatorRodriguez, L.F.-
dc.date2008-01-09T16:27:19Z-
dc.date2008-01-09T16:27:19Z-
dc.date2001-01-24-
dc.date.accessioned2017-01-31T00:59:40Z-
dc.date.available2017-01-31T00:59:40Z-
dc.identifierarXiv:astro-ph/0101435v2-
dc.identifierhttp://hdl.handle.net/10261/2667-
dc.identifier.urihttp://dspace.mediu.edu.my:8181/xmlui/handle/10261/2667-
dc.descriptionWe 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.-
dc.descriptionPeer reviewed-
dc.format156500 bytes-
dc.formatapplication/pdf-
dc.languageeng-
dc.relationPreprint-
dc.rightsopenAccess-
dc.subjectDust, extinction-
dc.subjectISM : HII regions-
dc.subjectISM : individual : Trifid-
dc.subjectStars : formation-
dc.titleDisks around Hot Stars in the Trifid Nebula-
dc.typePre-print-
Appears in Collections:Digital Csic

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