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• W2340358600 abstract "The ultraviolet-to-radio continuum spectral energy distributions are presented for all 75 galaxies in the Spitzer InfraredNearbyGalaxiesSurvey(SINGS).Aprincipalcomponentanalysisofthesampleshowsthatmostofthesample’sspectral variationsstem from twounderlying components,one representativeof agalaxywith alow infrared-toultraviolet ratio and one representative of a galaxy with a high infrared-to-ultraviolet ratio. The influence of several parameters ontheinfrared-to-ultraviolet ratio isstudied(e.g.,opticalmorphology,diskinclination, far-infrared color, ultraviolet spectral slope, and star formation history). Consistent with our understanding of normal star-forming galaxies,theSINGSsampleofgalaxies incomparisontomoreactivelystar-forming galaxies exhibitsalargerdispersion in the infrared-to-ultraviolet versus ultraviolet spectral slope correlation. Early-type galaxies, exhibiting low star formation rates and high optical surface brightnesses, have the most discrepant infrared-to-ultraviolet correlation. These results suggest that the star formation history may be the dominant regulator of the broadband spectral variations between galaxies. Finally, a new discovery shows that the 24 � m morphology can be a useful tool for parameterizing the global dust temperature and ultraviolet extinction in nearby galaxies. The dust emission in dwarf/irregular galaxies is clumpy and warm accompanied by low ultraviolet extinction, while in spiral galaxies there is typically a much larger diffuse component of cooler dust and average ultraviolet extinction. For galaxies with nuclear 24 � m emission, the dust temperature and ultraviolet extinction are relatively high compared to disk galaxies. Subject headingg galaxies: photometry — infrared: galaxies — infrared: ISM — ultraviolet: galaxies Online material: color figures" @default.
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• W2340358600 date "2007-01-01" @default.
• W2340358600 modified "2023-10-18" @default.
• W2340358600 title "AN ULTRAVIOLET-TO-RADIO BROADBAND SPECTRAL ATLAS OF NEARBY GALAXIES D. A. Dale, 1 A. Gil de Paz, 2 K. D. Gordon, 3 H. M. Hanson, 1 L. Armus, 4 G. J. Bendo, 5 L. Bianchi, 6 M. Block, 3" @default.
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