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2022PASP..134f4101Z - Publ. Astron. Soc. Pac., 134, part no 6, 4101-4101 (2022/June-1036)

Two-component TeV Emissions for Blazars.


Abstract (from CDS):

For blazars, its radio emissions are composed of two components. In the high energy bands, Tera-electronvolts (TeV; 1012electronvolts) emissions were detected from some blazars. Does the TeV emission also consist of two components? To investigate the TeV emission component, we compiled a sample of 51 TeV blazars with available radio core dominance parameters and applied a two-component (the beamed and the unbeamed) model to study the composition of blazar TeV emission. We obtained the core-dominance parameter at the TeV band through applying a relativistic beaming model, and found that the average TeV core-dominance parameter is log RTeVL=<3.12 ±2.83 >for 46 BL Lacs, and that is log RTeVFSRQ= <4.80 ±1.76 > for 5 FSRQs, which shows an indication that the core dominance parameter in BL Lacs is smaller than that in FSRQs. For the three subclasses of BL Lacs-high synchrotron peaked BL Lacs(HBLs), intermediate synchrotron peaked BL Lacs(IBLs) and low synchrotron peaked(LBLs), log RTeVHBL is smaller than log RTeVIBL and log RTeVLBL. Our results suggest that the blazar TeV emission from the core is thousands times stronger than from the extended region and the TeV emission is more core-dominated for the lower synchrotron peaked sources. In addition, a significant correlation between the TeV core-dominance parameter (log RTeV) and the radio one log Rradio) log RTeV = (2.56 ±0.08) log Rradio + 0.99, is obtained suggesting that the TeV emission is beamed and the TeV core-dominance parameter is an indicator of beaming effect at the TeV bands, and that the TeV emission has stronger beaming effect than the radio emission.

Abstract Copyright: © 2022. The Astronomical Society of the Pacific. All rights reserved.

Journal keyword(s): Active galactic nuclei - Blazars - Quasars - Gamma-rays

Simbad objects: 58

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