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A long hard look at MCG-6-30-15 with XMM-Newton

A. C. Fabian·S. Vaughan·K. Nandra·K. Iwasawa·D. R. Ballantyne·J. C. Lee·A. De Rosa·A. Turner·A. J. Young
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Abstract

We present first results from a 325 ks observation of the Seyfert 1 galaxy MCG-6-30-15 with XMM-Newton and BeppoSAX. The strong, broad, skewed iron line is clearly detected and is well characterised by a steep emissivity profile within 6r_g (i.e. 6GM/c^2) and a flatter profile beyond. The inner radius of the emission appears to lie at about 2r_g, consistent with results reported from both an earlier XMM-Newton observation of MCG-6-30-15 by Wilms et al. and part of an ASCA observation by Iwasawa et al. when the source was in a lower flux state. The radius and steep emissivity profile do depend however on an assumed incident power-law continuum and a lack of complex absorption above 2.5 keV. The blue wing of the line profile is indented, either by absorption at about 6.7 keV or by a hydrogenic iron emission line. The broad iron line flux does not follow the continuum variations in a simple manner.

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A. C. Fabian, S. Vaughan, K. Nandra, K. Iwasawa, D. R. Ballantyne, J. C. Lee, A. De Rosa, A. Turner, A. J. Young. 2002-06-06. A long hard look at MCG-6-30-15 with XMM-Newton. https://doi.org/10.1046/j.1365-8711.2002.05740.x

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