Abstract
Following the kinetic equation approach, we study the flare processes in blazars in the optical-to-X-ray region, considering energy dependent acceleration time-scale of electrons and synchrotron and adiabatic cooling as their dominant energy loss processes.
Similar content being viewed by others
References
Bhattacharyya, S., Sahayanathan, S. Kaul, C. L.in preparation
Drury, L. O. C. 1983,Rep. Prog. Phys.,46, 973.
Fossati, G.et al. 2000,ApJ,541, 153, 166.
Kataoka, J.et al. 1999,ApJ,514, 138.
Kirk, J. G., Riegler, F. M., Mastichiadis, A., 1998,A&A,333, 452.
Kusunose, M., Takahara, F, Li, H., astro-ph/0002137.
Maraschi, L. 1992, inVariability of Blazars, (ed.) E. Valtaoja & M. Valtonen (Cambridge: Cambridge Univ. Press),447
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Bhattacharyya, S., Sahayanathan, S. & Kaul, C.L. Effect of particle acceleration process on the flare characteristics of blazars. J Astrophys Astron 23, 95–99 (2002). https://doi.org/10.1007/BF02702471
Issue Date:
DOI: https://doi.org/10.1007/BF02702471