XMM-Newton Spectroscopy of the Seyfert 1.9 / NEL Galaxy NGC 7314

Details XMM-Newton Spectroscopy of the Seyfert 1.9 / NEL Galaxy NGC 7314 XMM-Newton Spectroscopy of the Seyfert 1.9 / NEL Galaxy NGC 7314

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002hrxs.confe...7b&link_type=abstract

High Resolution X-ray Spectroscopy with XMM-Newton and Chandra, Proceedings of the international workshop held at the Mullard Sp

Computer Science

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Scientific paper

Preliminary analysis of an XMM-Newton observation of NGC 7314 shows that rapid variability in the 0.2 - 12 keV flux of this object is not associated with spectral changes. A significant amount of warm absorption is required to explain the complexity of the X-ray spectrum at low energies. The continuum and Fe Kalpha line emission are best explained by a power law spectrum with reflection and fluorescence in cold gas at some distance from the active nucleus, far out in the accretion disk or in a molecular torus.

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