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The variable ROSAT X-ray spectrum of the BL Lac 0716+714

Astrophysics 2015-06-24 v1

Abstract

The BL Lac object 0716+714 is a powerful flat spectrum radio source detected by CGRO-EGRET at γ\gamma-ray energies. It has been observed for about 21000 s over two days by the X-ray telescope onboard the ROSAT satellite and strong flux and spectral variations have been detected. In the time scale of two days the source varied by a factor of 7\sim 7; during a sudden (1000\sim 1000 s) flux increase, the variation was 70\%. 0716+714 exhibits spectral variations related to source flux variability which may be attributed to a ``soft excess" component most prominent when the source was in a low state. The spectrum of 0716+714 steepened in the soft X-ray band when the flux decreased while in the hard X-ray band remained constant. A double power law model, representing steep synchrotron radiation at low energies and flat inverse Compton radiation above \sim 1 keV, best fits both the low and high state.

Keywords

Cite

@article{arxiv.astro-ph/9409068,
  title  = {The variable ROSAT X-ray spectrum of the BL Lac 0716+714},
  author = {M. Cappi and A. Comastri and S. Molendi and G. G. C. Palumbo and R. Della Ceca and T. Maccacaro},
  journal= {arXiv preprint arXiv:astro-ph/9409068},
  year   = {2015}
}

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