Emissive Mechanism on Spectral Variability of Blazars in High Frequencies

Details Emissive Mechanism on Spectral Variability of Blazars in High Frequencies Emissive Mechanism on Spectral Variability of Blazars in High Frequencies

2000-11-14

arxiv.org/abs/astro-ph/0011262v1

Astronomy and Astrophysics

Astrophysics

24 pages, 6 figures, Paper submitted to ApJ

Scientific paper

10.1086/321327

The new results of the evolution of the synchrotron peak for Mrk 421 are mostly likely related to the particle acceleration process. In order to account for the above results, we present a model of blazar variability during the flare in which the emission comes from accelerating electrons. A diffusion advection equation of the electron energy distribution is derived to calculate the spectrum and light curve of synchrotron radiation. We present that the observed shifts of the synchrotron peak moving to higher energies during the flare are caused by shock acceleration. The observed relation between changes in the fluxes at specified frequency ranges and shifts of the peak position is fitted to constrain the physical parameters of the dissipation region.

Affiliated with

Also associated with

No associations

Rating

Emissive Mechanism on Spectral Variability of Blazars in High Frequencies 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 Emissive Mechanism on Spectral Variability of Blazars in High Frequencies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Emissive Mechanism on Spectral Variability of Blazars in High Frequencies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-351339