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arXiv · astro-ph/9711145

BeppoSAX observation of NGC 7674: a new reflection-dominated Seyfert 2 galaxy

G. Malaguti·G. G. C. Palumbo·M. Cappi·A. Comastri·C. Otani·M. Matsuoka·M. Guainazzi·L. Bassani·F. Frontera
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Abstract

The Seyfert 2 galaxy NGC 7674 has been observed within the BeppoSAX Core Programme with the onboard narrow field instruments between 0.1 and 100 keV. The broad-band spectrum shows four most relevant spectral components: a) a soft excess below ~2 keV; b) a prominent (EW~1 keV) Fe line; c) a flat (Gamma~1.1) 2-10 keV continuum; d) a 4.5sigma detection above 13 keV. The flat power law spectrum can be very well explained within the current AGN unified models assuming a steep (Gamma~2) intrinsic spectrum scattered by warm gas for the low energy band and totally reflected by optically thick cold matter (plausibly a molecular torus) for the high energy band. The case of NGC 7674 adds to the increasing number of so called "Compton-thick" Seyfert 2 galaxies in which the direct emission is totally absorbed and the X-ray luminosity is thus at least one or two orders of magnitude larger than what inferred from the observed flux.

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G. Malaguti, G. G. C. Palumbo, M. Cappi, A. Comastri, C. Otani, M. Matsuoka, M. Guainazzi, L. Bassani, F. Frontera. 1997-11-13. BeppoSAX observation of NGC 7674: a new reflection-dominated Seyfert 2 galaxy. https://arxiv.org/abs/astro-ph/9711145

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