Abstract
We obtain an approximate analytical solution using δ approximate calculation on the traditional one-zone synchrotron self-Compton (SSC) model. In this model, we describe the electron energy distribution by a broken power-law function with a sharp cut-off, and non-thermal photons are produced by both synchrotron and inverse Compton scattering of synchrotron photons. We calculate the radiation energy spectrum of electrons by the δ function. We apply this model to the multi-wavelength Spectral Energy Distributions (SED) of the 3C 273 in different states, and obtain excellent fits to the observed spectra of this source.
Similar content being viewed by others
References
Abdo, A. A., Ackermann, M., Ajello, M. et al. 2010, Astrophys. J., 714, 73.
Kang, S. J., Huang, B. R., Kang, T. et al. 2012, Chinese Astron. Astrophys., 36, 115.
Rybicki, G. B., Lightman, A. P. 1979, Radiative Processes in Astrophys., New York.
Acknowledgements
This work is supported by NSFC under grants 11178019, 11103003 and 11133005.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Kang, S.J., Zheng, Y.G. & Wu, Q. Delta-function Approximation SSC Model in 3C 273. J Astrophys Astron 35, 385–386 (2014). https://doi.org/10.1007/s12036-014-9236-6
Published:
Issue Date:
DOI: https://doi.org/10.1007/s12036-014-9236-6