Similar radiation mechanism in gamma-ray bursts and blazars: evidence from two luminosity correlations
arXiv:1403.7857 · doi:10.1088/2041-8205/786/1/L8
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 and correlations, where is defined as the broadband spectral slope in radio-to-X-ray bands, and 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.
12 pages, 2 figures, 1 table. Accepted for publication by ApJL
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Cited by in corpus (8)
- Gamma-ray Burst Cosmology
- A Comprehensive Power Spectral Density Analysis of Astronomical Time Series. II. The Swift/BAT Long Gamma-Ray Bursts
- Universal Behavior of X-ray Flares from Black Hole Systems
- Distributions of Gamma-Ray Bursts and Blazars in the Plane and Possible Implications for their Radiation Physics
- Observable Emission Features of Black Hole GRMHD Jets on Event Horizon Scales
- A universal scaling law of black hole activity including gamma-ray bursts
- A Universal Energy Relation between synchrotron and Synchrotron Self-Compton radiation in GRBs and Blazars
- relation in Active Galactic Nucleus Jets and Implication for the physical origin of the relation of Gamma-Ray Bursts