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X-Ray Emission from BL LAC Objects: Comparison to the Synchrotron Self-Compton Models

Published online by Cambridge University Press:  14 August 2015

Daniel A. Schwartz
Affiliation:
Harvard/Smithsonian Center for Astrophysics
Greg Madejski
Affiliation:
Harvard/Smithsonian Center for Astrophysics
William H.-M. Ku
Affiliation:
Columbia Astrophysics Laboratory

Extract

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As one part of our joint study of the X-ray properties of BL Lac objects, we compare the measured X-ray flux densities with those predicted using the synchrotron self-Compton (SSC) formalism (Jones ET AL. 1974). Naive application of the formalism predicts X-ray fluxes from 10−3 to 105 those observed. We therefore ask what we can learn by simply assuming the SSC mechanism, and looking for ways to reconcile the observed and measured X-ray fluxes. This paper reports our investigation of beaming factors due to relativistic ejection of a radiation source which is isotropic in its own rest frame. We conclude that large Lorentz factors, Γ ≳ 10, do not apply to BL Lac objects as a class.

Type
Research Article
Copyright
Copyright © Reidel 1982 

References

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