2002/09/30 by Richard J. Tuffs, Tuffs, Richard J., C. C. Popescu +2
Chemistry · Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Spectroscopy and Laser Applications #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0209622
7 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
arxiv created 2002/09/30 · openalex publication_date 2002/09/30 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We 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.