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Thermal infrared and nonthermal radio - Remarkable correlation in disks of galaxies

Helou, G., Soifer, B. T., Rowan-Robinson, M.·1985·The Astrophysical Journal

Abstract

A tight, linear correlation is established between the far-infrared flux measured by IRAS and the nonthermal radio flux density (at 1.4 GHz) from disks of spiral galaxies. This correlation defines a ratio of infrared to radio fluxes that is characteristic of star formation activity. Galaxies with nuclear starbursts seem to follow the correlation. If the far-infrared is reradiated luminosity from young massive stars, then the supernova remnants alone account for less than 10 percent of the radio emission. These results indicate a close coupling between dust heating and cosmic-ray generation and confinement in a wide range of conditions.

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Metadata

Authors
Helou, G., Soifer, B. T., & Rowan-Robinson, M.
Venue
The Astrophysical Journal
Published
1985-11
Volume
298
Pages
L7
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2025969090
Cited by
942
References
0
FWCI
2.57
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Thermal infrared and nonthermal radio - Remarkable correlation in disks of galaxies. https://app.cochat.ai/papers/10.1086/184556
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Helou, G., Soifer, B. T., & Rowan-Robinson, M. (1985). Thermal infrared and nonthermal radio - Remarkable correlation in disks of galaxies. The Astrophysical Journal. https://doi.org/10.1086/184556

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