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Relation between $γ$-rays and emission lines for the $γ$-ray loud blazars

J. H. Fan
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Abstract

The relation between the $γ$-ray and the emission line luminosities for a sample of 36 $γ$-ray loud blazars is investigated; an apparent correlation between them, $L_γ \propto L_{Line}^{0.69\pm0.11}$, with a correlation coefficient $r=0.741$ and a chance probability of $p = 1.9\times10^{-6}$, is found. It is found, however, that there is no intrinsic correlation between them: the apparent correlation is due to the redshift dependence in a flux-limited sample. Thus no evidence is found to support the argument that the up-scattered soft photons are from the broad emission lines. Our analysis does not conflict with the SSC model. The disk-jet symbiosis and radio/$γ$-ray correlation found in the literature are also discussed. The radio/$γ$-ray correlation may be an apparent correlation caused by the boosting effect since both bands are strongly beamed.

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J. H. Fan. 2000-07-21. Relation between $γ$-rays and emission lines for the $γ$-ray loud blazars. https://arxiv.org/abs/astro-ph/0007326

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