Spectrum of the Accretion Disk Near the Rotating Black Hole

Details Spectrum of the Accretion Disk Near the Rotating Black Hole Spectrum of the Accretion Disk Near the Rotating Black Hole

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.2265r&link_type=abstract

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

Physics

Scientific paper

Recent observations of Seyfert galaxies, carried out by ASCA and RXTE seem to indicate that the broad iron Kα line (6.4 keV) takes its origin in the innermost area of the accretion disk around a supermassive black hole. A spectrum of a solitary emission line has been simulated. It is shown that the characteristic two-peak line profile with the sharp edges arises at a large distance (r ≈ (3 - 10)rg) or large inclination angle. The inner regions emit the line, which is observed at the infinity with one maximum and extremely wide red wing. The disk spectrum is simulated then as a sum of the thin rings spectra. It is shown also that the angular momentum a = J/M is a difficult parameter for the immediate measurements.

Affiliated with

Also associated with

No associations

Rating

Spectrum of the Accretion Disk Near the Rotating Black Hole does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectrum of the Accretion Disk Near the Rotating Black Hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrum of the Accretion Disk Near the Rotating Black Hole will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1168784