New Results from Observations of Massive Star Formation in the Mid-Infrared with Large Aperture Telescopes

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dc.creatorDe Buizer, James M.
dc.date2006-10-18
dc.date.accessioned2026-07-07T07:27:01Z
dc.date.available2026-07-07T07:27:01Z
dc.descriptionThanks to the high spatial resolution afforded by 8-10m class telescopes, we are beginning to learn that some sources are extended in their mid-infrared emission because of dusty outflows or heated outflow cavity walls. Therefore one must be extremely careful in interpreting the nature of extended mid-infrared sources (i.e. just because it is extended does not automatically mean it is a disk!).
dc.descriptionTo appear in proceedings of the conference "First Light Science with the GTC", eds. R. Guzman, C. Packham & J.M. Rodriguez Espinosa (RMAA Conf. Ser.), in press; also available at http://www.ctio.noao.edu/~debuizer
dc.identifierhttps://arxiv.org/abs/astro-ph/0610541
dc.identifierhttp://arxiv.org/abs/astro-ph/0610541
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117237
dc.subjectAstrophysics
dc.titleNew Results from Observations of Massive Star Formation in the Mid-Infrared with Large Aperture Telescopes
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