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Hardening of the X-ray spectrum and signature of Fe abundance in Mrk 501 based on the filamentary jet model

Published online by Cambridge University Press:  25 July 2014

Yasuko S. Honda
Affiliation:
Kinki University Technical College, Kasugaoka 7-1, Nabari, Mie, 518-0459, Japan email: honda@tse.kutc.ac.jp
Mitsuru Honda
Affiliation:
Plasma Astrophysics Laboratory, Institute for Global Science, Kumano, Mie, 519-4327, Japan
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Abstract

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We evaluate the synchrotron spectrum of Mrk 501 based on our filamentary jet model. Integrating the contribution from the magnetic fields induced by numerous current filaments with various transverse sizes, we reproduce the observed hardening of the spectrum around X-rays. It is found that the spectral change during 1997-1998 can be explained by the evolution of turbulence. We also propose that the observed dip around 80 keV is attributed to bound-free absorption by Fe atoms, which implies the abundance of heavy nuclei at the tip of the jet.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

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