Model of Radiating Annuli Near Black Holes for Iron Kα Line Profile Interpretations

Details Model of Radiating Annuli Near Black Holes for Iron Kα Line Profile Interpretations Model of Radiating Annuli Near Black Holes for Iron Kα Line Profile Interpretations

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1069z&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

X-ray observations of microquasars and Seyfert galaxies reveal the broad emission lines in their spectra, which can arise in the innermost parts of accretion disks. We consider a radiating annulus model to simulate spectral line shapes. Recently Muller & Camenzind (2004) presented results of their calculations and classified different types of spectral line shapes and described their origin. We clarified their results and showed that triangular spectral lines could arise for nearest annuli and high inclination angles. We discussed a possibility of appearance of narrow spectral line shapes as a result of spiralling evolution of matter along quasi-circular orbits.

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