The 10-200 MU M spectral energy distribution of the prototype narrow-line X-ray galaxy NGC 7582
We present the spectral energy distribution (SED) between 10 and 200 mu m obtained for the prototype narrow-line X-ray galaxy NGC 7582 with ISOPHOT, the photometer on board the Infrared Space Observatory. The emission is spatially extended and we separated for the first time the nuclear and extranuclear infrared SEDs. The nuclear luminosity (L_IR ~
Radovich, M. et al.
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1999