Abstract
The importance of the far infrared emission to the study of stellar populations in galaxies is that in the local universe a comparable amount of energy emerges in the far infrared as in the uv-optical region [1-2]. IRAS has now made available to us far infrared fluxes for over 20,000 galaxies.
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Persson, C.J. (1987). Star Formation in Disks: IRAS Results. In: Faber, S.M. (eds) Nearly Normal Galaxies. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-4762-3_5
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DOI: https://doi.org/10.1007/978-1-4612-4762-3_5
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