Abstract.
We present temporal and spectral analysis of the X-ray bright blazar PKS 2155-304 observed with BeppoSAX. Power density spectra show strong red noise feature with steep slope of \(\sim 2-3\). Structure functions suggest typical timescale of \(\sim 0.5\) days. Inter-band time lags differ from flare to flare. Peak energies of synchrotron component increase with increasing flux, and complexities of spectral evolution are detected. The implications of our results are discussed in the context of synchrotron cooling model of relativistic electrons accelerated through internal shocks taking place in the jet.
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Zhang, Y.H. et al. X-Ray Variability of Blazar PKS 2155-304: Probing the Dynamics of the Jet. In: Gilfanov, M., Sunyeav, R., Churazov, E. (eds) Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10856495_47
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DOI: https://doi.org/10.1007/10856495_47
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Publisher Name: Springer, Berlin, Heidelberg
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