Far-infrared Emission from Dust in Normal Galaxies

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dc.creatorTuffs, Richard J.
dc.creatorPopescu, Cristina C.
dc.date2002-09-30
dc.date.accessioned2026-07-07T02:05:29Z
dc.date.available2026-07-07T02:05:29Z
dc.descriptionWe review the morphological and spectral energy distribution characteristics of the dust continuum emission (emitted in the 40-200 micron spectral range) from normal galaxies, as revealed by detailed ISOPHOT mapping observations of nearby spirals and by ISOPHOT observations of the integrated emissions from representative statistical samples in the local universe.
dc.description7 pages with 5 figures included (eps format); invited review talk held at the ESA Workshop ``Exploiting the ISO Data Archive. Infrared Astronomy in the Internet Age'', Siguenza, Spain 24-27 June, 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0209622
dc.identifierhttp://arxiv.org/abs/astro-ph/0209622
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5116
dc.subjectAstrophysics
dc.titleFar-infrared Emission from Dust in Normal Galaxies
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