The Iron Line Production by MHD Shock in Kerr Geometry

Details The Iron Line Production by MHD Shock in Kerr Geometry The Iron Line Production by MHD Shock in Kerr Geometry

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.2332t&link_type=abstract

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

Physics

Scientific paper

From the resent observations of iron line of Seyfert galaxies MCG-6-30-15, there are at least two states in line profiles. We can expect that the two states would be cased by the variability of the location of shocked accreting plasmas, which would emit hard X-ray, in a black-hole magnetosphere. I discuss the conditions for trans-fast magnetosonic accretions, and construct a shock formation model.

Affiliated with

Also associated with

No associations

Rating

The Iron Line Production by MHD Shock in Kerr Geometry 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 The Iron Line Production by MHD Shock in Kerr Geometry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Iron Line Production by MHD Shock in Kerr Geometry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1168852