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The mid-infrared spectra of normal galaxies.

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dc.contributor.author Helou, G. en_US
dc.contributor.author Lu, N. en_US
dc.contributor.author Werner, M. en_US
dc.contributor.author Malhotra, S. en_US
dc.contributor.author Silbermann, N. en_US
dc.date.accessioned 2004-09-23T17:34:19Z
dc.date.available 2004-09-23T17:34:19Z
dc.date.issued 2000-03 en_US
dc.identifier.citation Astrophysical journal, Vol. 532, No. 1, 2000, pp. L21-L24 en_US
dc.identifier.citation Pasadena, CA USA en_US
dc.identifier.clearanceno 00-0315 en_US
dc.identifier.uri http://hdl.handle.net/2014/13938
dc.description.abstract The mid-infrared spectra (2.5-5 and 5.7-11.6 mu m) obtained by ISOPHOT reveal the interstellar medium emission from galaxies powered by star formation to be strongly dominated by the aromatic features at 6.2, 7.7, 8.6, and 11.3 mu m. Additional emission appears in between the features, and an underlying continuum is clearly evident at 3-5 mu m. This continuum would contribute about a third of the luminosity in the 3-13 mu m range. The features together carry 5%-30% of the 40-120 mu m. range.FIR) luminosity. en_US
dc.format.extent 77824 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Mid-infrared spectra spectrophotometry en_US
dc.title The mid-infrared spectra of normal galaxies. en_US


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