Branduardi-Raymont, G;
Sako, M;
Kahn, SM;
Brinkman, AC;
Kaastra, JS;
Page, MJ;
(2001)
Soft X-ray emission lines from a relativistic accretion disk in MCG-6-30-15 and Mrk 766.
ASTRON ASTROPHYS
, 365
(1)
L140 - L145.
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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 Angstrom 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.
Type: | Article |
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Title: | Soft X-ray emission lines from a relativistic accretion disk in MCG-6-30-15 and Mrk 766 |
Open access status: | An open access version is available from UCL Discovery |
Keywords: | black hole physics, accretion, accretion disks, line : formation, galaxies : individual : MCG-6-30-15, galaxies : individual : Mrk 766, X-rays : galaxies, ACTIVE GALACTIC NUCLEI, BLACK-HOLE, GALAXIES |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
URI: | https://discovery-pp.ucl.ac.uk/id/eprint/9261 |
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