arXiv · 1403.7857
Similar radiation mechanism in gamma-ray bursts and blazars: evidence from two luminosity correlations
Abstract
Active galactic nuclei (AGNs) and gamma-ray bursts (GRBs) are powerful astrophysical events with relativistic jets. In this Letter the broadband spectral properties are compared between GRBs and the well-observed blazars. The distribution of GRBs are consistent with the well-known blazar sequence including the $νL_ν(5\rm GHz)-α_{\rm RX}$ and $νL_ν(5\rm GHz)-ν_{\rm peak}$ correlations, where $α_{\rm RX}$ is defined as the broadband spectral slope in radio-to-X-ray bands, and $ν_{\rm peak}$ is defined as the spectral peak frequency. Moreover, GRBs occupy the low radio luminosity end of these sequences. These two correlations suggest that GRBs could have a similar radiation process with blazars both in the prompt emission and afterglow phases, i.e., synchrotron radiation.
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F. Y. Wang, S. X. Yi, Z. G. Dai. 2014-03-31. Similar radiation mechanism in gamma-ray bursts and blazars: evidence from two luminosity correlations. https://doi.org/10.1088/2041-8205%2F786%2F1%2Fl8
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