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Delta-function Approximation SSC Model in 3C 273

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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.

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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.

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Acknowledgements

This work is supported by NSFC under grants 11178019, 11103003 and 11133005.

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Correspondence to S. J. Kang.

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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

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  • DOI: https://doi.org/10.1007/s12036-014-9236-6

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