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Soft X-ray emission lines from a relativistic accretion disk in MCG -6-30-15 and Mrk 766

G. Branduardi-Raymont·M. Sako·S. M. Kahn·A. C. Brinkman·J. S. Kaastra·M. J. Page
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Abstract

XMM-Newton Reflection Grating Spectrometer (RGS) spectra of the Narrow Line Seyfert 1 galaxies MCG -6-30-15 and Mrk 766 are physically and spectroscopically inconsistent with standard models comprising a power-law continuum absorbed by either cold or ionized matter. We propose that the remarkably similar features detected in both objects in the 5 - 35 A band are H-like oxygen, nitrogen, and carbon emission lines, gravitationally redshifted and broadened by relativistic effects in the vicinity of a Kerr black hole. We discuss the implications of our interpretation, and demonstrate that the derived parameters can be physically self-consistent.

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G. Branduardi-Raymont, M. Sako, S. M. Kahn, A. C. Brinkman, J. S. Kaastra, M. J. Page. 2000-11-08. Soft X-ray emission lines from a relativistic accretion disk in MCG -6-30-15 and Mrk 766. https://doi.org/10.1051/0004-6361%3A20000209

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