Physics
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..241m&link_type=abstract
The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,
Physics
Scientific paper
We investigate the classification of Active Galactic nuclei (AGN) of powerful jets FR I and FR II. We use a steady axisymmetric self-similar model of relativistic magnetohydrodynamics (GRMHD) outflows originating at the hot coronal magnetosphere of a Schwarzschild black hole and surrounding accretion disk. We demonstrate that the differences between the jets of FR II and FR I are related to the rotation of corona. When the rotation slows down and deviates strongly form the Keplerian rotation, the Poyting flux injected in the jet decreases. As result, the efficiency of the magnetic pinching decreases and influence of the external medium in the jet increases, so the proprieties of jets change from that of FR II to FR I.
No associations
LandOfFree
Formation and Collimation of Relativistic Jets -- Application to the Classification of FR I and FR II Radio Galaxies 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 Formation and Collimation of Relativistic Jets -- Application to the Classification of FR I and FR II Radio Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation and Collimation of Relativistic Jets -- Application to the Classification of FR I and FR II Radio Galaxies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-953735