Linking {\it Fermi} blazars and radio galaxies through accretion and jet radiation mechanisms
Xu-Hong Ye, Ranieri D. Baldi, Wen-Xin Yang, Jing-Tian Zhu, Denis Bastieri, Rumen S. Bachev, Anton A. Strigachev, and Jun-Hui Fan

TL;DR
This study supports a unified model linking blazars and radio galaxies through their accretion states and jet emission mechanisms, based on statistical analysis of their gamma-ray properties and classifications.
Contribution
It provides new evidence for a unified accretion-ejection scenario, connecting aligned and misaligned radio-loud AGNs via optical emission-line classifications.
Findings
HERGs have higher gamma-ray luminosities and softer spectra, similar to FSRQs.
LERGs exhibit lower luminosities and harder spectra, akin to BL Lacs.
Distinct accretion states correlate with different emission mechanisms (EC vs. SSC).
Abstract
Based on the classical unification, blazars, namely BL Lacertae objects (BL Lacs) and flat-spectrum radio quasars (FSRQs), are believed to correspond with radio galaxies when observed at small jet viewing angles. In this paper, we aim to compile a sample of Fermi blazars and radio galaxies to provide new insights towards a unified accretion and ejection scenario between aligned and misaligned radio-loud active galactic nuclei (AGNs), by considering their optical emission-line classifications (low- and high-excitation radio galaxies, LERGs, HERGs), which are more representative of their accretion states. We adopted statistical analyses of accretion properties and high-energy beaming patterns for both Fermi blazars and radio galaxies to investigate a unified accretion-ejection scenario. In the gamma-ray luminosity-photon index plane, HERGs populate the region of higher luminosities and…
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