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XMM-EPIC observation of MCG-6-30-15: Direct evidence for the extraction of energy from aspinning black hole?

Joern Wilms·Christopher S. Reynolds·Mitchell C. Begelman·James Reeves·Silvano Molendi·Ruediger Stuabert·Eckhard Kendziorra
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Abstract

We present XMM-Newton European Photon Imaging Camera (EPIC) observations of the bright Seyfert 1 galaxy MCG-6-30-15, focusing on the broad Fe K$α$ line at ~6keV and the associated reflection continuum, which is believed to originate from the inner accretion disk. We find these reflection features to be extremely broad and red-shifted, indicating its origin from the very most central regions of the accretion disk. It seems likely that we have caught this source in the ``deep minimum'' state first observed by Iwasawa et al. (1996). The implied central concentration of X-ray illumination is difficult to understand in any pure accretion disk model. We suggest that we are witnessing the extraction and dissipation of rotational energy from a spinning black hole by magnetic fields connecting the black hole or plunging region to the disk.

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Joern Wilms, Christopher S. Reynolds, Mitchell C. Begelman, James Reeves, Silvano Molendi, Ruediger Stuabert, Eckhard Kendziorra. 2001-10-23. XMM-EPIC observation of MCG-6-30-15: Direct evidence for the extraction of energy from aspinning black hole?. https://doi.org/10.1046/j.1365-8711.2001.05066.x

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