1. The correlation between γ $\gamma$ -photon energy and synchrotron peak frequency for Fermi BL Lac objects
- Author
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Yi Liu, Jiang-He Yang, Yue-Lian Zhang, Y. H. Yuan, RuShu Yang, M. X. Tuo, Jun-Hui Fan, and J. J. Nie
- Subjects
Physics ,Photon ,Active galactic nucleus ,010308 nuclear & particles physics ,Astrophysics::High Energy Astrophysical Phenomena ,Gamma ray ,Gamma photon ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Photon energy ,01 natural sciences ,Synchrotron ,law.invention ,Space and Planetary Science ,law ,0103 physical sciences ,Atomic physics ,010303 astronomy & astrophysics ,Energy (signal processing) ,Fermi Gamma-ray Space Telescope - Abstract
In this paper, the average energy of the $\gamma$ -photon ( $E_{\mathrm {a},\mathrm{ph}}$ ) is calculated and the correlation between $\log E_{\mathrm{a},\mathrm{ph}}$ and the logarithm of the synchrotron peak frequency ( $\log\nu_{\mathrm{p}}$ ) is discussed for a sample of 620 BL Lac objects. The results show that there exists a positive correlation between the $\gamma$ -photon energy and the synchrotron peak frequency for BL Lac objects, which implies that the $\gamma$ -ray emissions are related to the low-energy emissions of radio to X-ray bands, and the high energetic $\gamma$ -ray emissions are only partially from the synchrotron self-Compton process (SSC) for BL Lac objects.
- Published
- 2017
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