Organized Criticalitly and Variability of Structure with Data from MCG -6-30-15

Details Organized Criticalitly and Variability of Structure with Data from MCG -6-30-15 Organized Criticalitly and Variability of Structure with Data from MCG -6-30-15

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.5704s&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #57.04; Bulletin of the American Astronomical Society, Vol. 30, p.1333

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The X-ray spectral features of Seyfert I nuclei, are presumably due to the reprocessing of emission from hot (relativistic) plasma by a {stationary} thin accretion disk near a black hole, and a {stationary} optically thin warm absorber in the line of sight. The non-variable structure is inconsistent with the high amplitude non-linear light-curve in some Seyferts, and the manner in which the spectrum varies in others. Several non-stationary configurations were recently proposed in theoretical work on self-organized criticality (SOC) in near-Eddington accreting sources. It is shown that the SOC models are consistent with the light-curve and spectral variability and of Seyfert I MCG -6-30-15. Preliminary analysis of other Seyferts gives similar results. It is also shown that the {gravitational} redshift of the Fe K line is needed in non-stationary geometries.

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