An XMM-Newton observation of the Narrow Line Seyfert 1 Galaxy, Markarian 896

K. L. Page; P. T. O'Brien; J. N. Reeves; A. A. Breeveld

doi:10.1046/j.1365-8711.2003.06403.x

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arXiv · astro-ph/0301152

An XMM-Newton observation of the Narrow Line Seyfert 1 Galaxy, Markarian 896

K. L. Page·P. T. O'Brien·J. N. Reeves·A. A. Breeveld

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Abstract

XMM-Newton observations of the NLS1 Markarian 896 are presented. Over the 2-10 keV band, an iron emission line, close to 6.4 keV, is seen. The line is just resolved and has an equivalent width of ~170 eV. The broad-band spectrum is well modelled by a power law slope of gamma ~ 2.03, together with two blackbody components to fit the soft X-ray excess. Using a more physical two-temperature Comptonisation model, a good fit is obtained for an input photon distribution of kT ~ 60eV and Comptonising electron temperatures of ~0.3 and 200 keV. The soft excess cannot be explained purely through the reprocessing of a hard X-ray continuum by an ionised disc reflector.

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K. L. Page, P. T. O'Brien, J. N. Reeves, A. A. Breeveld. 2003-01-09. An XMM-Newton observation of the Narrow Line Seyfert 1 Galaxy, Markarian 896. https://doi.org/10.1046/j.1365-8711.2003.06403.x

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