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Symmetric and triangle-shaped variability of blazars

Published online by Cambridge University Press:  24 March 2015

Kenji Yoshida
Kenji Yoshida*
Affiliation:
College of Systems Engineering and Science, Shibaura Institute of Technology, 307 Fukasaku, Minuma-ku, Saitama 337-8570, Japan email: [email protected]
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Abstract

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Symmetric and triangle-shaped flux variability in X-ray and gamma-ray light curves is observed from many blazars. We derived the X-ray spectrum changing in time by using a kinetic equation of high energy electrons. Giving linearly changing the injection of low energy electrons into accelerating and emitting region, we obtained the preliminary results that represent the characteristic X-ray variability of the linear flux increase with hardening in the rise phase and the linear decrease with softening in the decay phase.

Keywords

galaxies: jetsBL Lacertae objects: generalX-rays: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S313: Extragalactic jets from every angle , September 2014 , pp. 97 - 98
Copyright
Copyright © International Astronomical Union 2015 

References

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