Extended nonnuclear infrared emission from Seyfert galaxies
The IRAS observations of well-known Seyfert galaxies have been studied in comparison with previously published ultraviolet and mid-infrared data. The mid- and far-infrared emission from Seyfert galaxies has an important extended component. Moreover, the UV-optical continuum is insufficient to account for the far-infrared emission via dust
Rodriguez-Espinosa, J. M. et al.
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