arXiv Analytics

Sign in

arXiv:astro-ph/9901324AbstractReferencesReviewsResources

Variability in Blazars

Charles D. Dermer

Published 1999-01-22Version 1

The kinetic energy of bulk relativistic plasma ejected from the central engine of blazars is converted into nonthermal particle energy in the comoving frame through a process of sweeping up material from the surrounding medium. The resulting deceleration of the bulk plasma introduces a number of effects which must be included in blazar modeling. For example, the varying Doppler factor means that model fits must employ time integrations appropriate to the observing times of the detectors. We find that the ratio of the peak synchrotron fluxes reached at two different photon energies is largest when viewing along the jet axis, and becomes smaller at large angles to the jet axis. This effect is important in studies of the statistics of jet sources. Variability due either to bulk plasma deceleration or radiative cooling must be distinguished in order to apply recently proposed tests for beaming from correlated X-ray and TeV observations. The blast-wave physics developed to analyze these problems implies that most of the energy injected in the comoving frame is originally in the form of nonthermal hadrons. Because plasmoid deceleration can produce rapid variability due to a changing Doppler factor, arguments against hadronic blazar models related to the long radiative cooling time scale of hadrons are not compelling.

Comments: 13 pages, 3 figures,Invited talk at VERITAS Workshop on TeV Astrophysics of Extragalactic Sources, Cambridge, MA, Oct. 23-24, 1998. In press, Astroparticle Physics, ed. M. Catanese, J. Quinn, T. Weekes
Journal: Astropart.Phys. 11 (1999) 1-9
Categories: astro-ph
Related articles: Most relevant | Search more
arXiv:astro-ph/0003282 (Published 2000-03-20)
Hadronic blazar models and correlated X-ray/TeV flares
arXiv:astro-ph/0412383 (Published 2004-12-15)
VLBA Polarization Observations of Markarian 421 After a Gamma-Ray High State
arXiv:astro-ph/0506453 (Published 2005-06-20, updated 2005-08-17)
Prompt and afterglow early X-ray phases in the comoving frame. Evidence for Universal properties?