Highly ionized Fe K α emission lines from the LINER galaxy M 81 ⋆

Abstract

We present spectral and timing results from a long (130 ks) XMM-Newton EPIC observation of the nucleus of the Seyfert/LINER galaxy M 81. During the observation the X-ray flux varied by 20%, but there was no significant change in spectral shape. The 2–10 keV spectrum is well described by a power law continuum and three narrow Fe Kα emission lines at 6.4, 6.7… (More)

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