NGC 3576 IRS 1 in the Mid Infrared

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dc.creatorBarbosa, Cassio
dc.creatorDamineli, Augusto
dc.creatorBlum, Robert
dc.creatorConti, Peter
dc.date2002-08-17
dc.date.accessioned2026-07-07T02:04:43Z
dc.date.available2026-07-07T02:04:43Z
dc.descriptionWe present the results of high-resolution mid-infrared observations of the source NGC 3576 IRS 1. Near diffraction-limited images were taken at the Gemini South Observatory through OSCIR's filters N, 7.9, 9.8, 12.5 and IHW18. The source IRS 1 was resolved into 3 sources for the first time at mid-infrared wavelengths. For each source we constructed the SED from 1.25 to 18 microns, as well the color temperature and the spatial distribution of the dust in the region. The optical depth of the silicate absorption feature at 9.8 microns is presented also.
dc.description5 pages, 6 figures. To appear in 'Galactic Star Formation Across the Stellar Mass Spectrum' eds. J.M. De Buizer and N.S. van der Blieke (ASP Con. Series, 2002)
dc.identifierhttps://arxiv.org/abs/astro-ph/0208331
dc.identifierhttp://arxiv.org/abs/astro-ph/0208331
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4868
dc.subjectAstrophysics
dc.titleNGC 3576 IRS 1 in the Mid Infrared
dc.typetext

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