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Nature of 60 micron emission in 3C47, 3C207 and 3C334

Ilse M. van Bemmel·Peter D. Barthel·Min S. Yun
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Abstract

We try to explain the unusually high far-infrared emission seen by IRAS in the double-lobed radio-loud quasars 3C47, 3C207 and 3C334. High resolution cm--mm observations were carried out to determine their radio core spectra, which are subsequently extrapolated to the far-infrared in order to determine the strength of the synchrotron far-infrared emission. The extrapolated flux densities being considerably lower than the observed values, a significant nonthermal far-infrared component is unlikely in the case of 3C47 and 3C334. However, this component could be responsible for the far-infrared brightness of 3C207. Our analysis demonstrates that nonthermal emission cannot readily account for the difference between quasars and radio galaxies in the amount of their far-infrared luminosity. On the other hand, a significant role for this mechanism is likely; full sampling of the mm-submm spectral energy distributions is needed to address the issue quantitatively.

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Ilse M. van Bemmel, Peter D. Barthel, Min S. Yun. 1998-03-18. Nature of 60 micron emission in 3C47, 3C207 and 3C334. https://arxiv.org/abs/astro-ph/9803210

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