The 10 - 200 μ m spectral energy distribution of the prototype

Abstract

We present the spectral energy distribution (SED) between 10 and 200 μm 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 (LIR ∼ 4.5×10 10 L… (More)

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@inproceedings{Radovich1999The1, title={The 10 - 200 μ m spectral energy distribution of the prototype}, author={Mario Radovich and Ulrich Klaas and Dietrich Lemke}, year={1999} }