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Related papers: Jet Power of Jetted Active Galactic Nuclei: Implic…

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Narrow-line Seyfert 1 galaxies (NLS1s), a subclass of active galactic nuclei (AGNs) at early stage of accretion process, are also found to host relativistic jets. However, currently known jetted NLS1s are rare. The majority of NLS1s are…

Astrophysics of Galaxies · Physics 2024-02-23 Xu-Liang Fan

The composition and energy dissipation in jets are two of the fundamental questions of jet physics that are not fully understood. In this paper, we attempt to constrain the composition, magnetization as well as radiative efficiency for…

Astrophysics of Galaxies · Physics 2018-07-25 Xu-Liang Fan , Qingwen Wu , Neng-Hui Liao

We investigate the relation between the two modes of outflow (wind and jet) in radio-loud active galactic nuclei (AGN). For this study we have carried out a systematic and homogeneous analysis of XMM-Newton spectra of a sample of 16…

High Energy Astrophysical Phenomena · Physics 2019-05-08 Missagh Mehdipour , Elisa Costantini

Active galactic nuclei (AGNs) are known to cover an extremely broad range of radio luminosities and the spread of their radio-loudness is very large at any value of the Eddington ratio. This implies very diverse jet production efficiencies…

Astrophysics of Galaxies · Physics 2017-11-07 D. Kozieł-Wierzbowska , G. Stasińska , N. Vale Asari , M. Sikora , E. Goettems , A. Wójtowicz

We constrain the behavior of the radio luminosity function (RLF) of two classes of active galactic nuclei (AGN) namely AGN of low radio power (LRP) and BL Lac objects. The extrapolation of the observed steep RLFs to low power predicts a…

Astrophysics of Galaxies · Physics 2015-06-24 Alessandro Capetti , Claudia M. Raiteri

Typical blazars seem to be associated with FR I and FR II radio galaxies and radio-loud quasars. However, what happens at lower powers? Do blazars exist in low-luminosity AGN or do they exist in radio-quiet AGN? A recent detection of…

Astrophysics · Physics 2007-05-23 Heino Falcke , Sera Markoff , Peter L. Biermann

This paper presents a study of the redshift evolution of radio-loud active galactic nuclei (AGN) as a function of the properties of their galaxy hosts in the Bo\"otes field. To achieve this we match low-frequency radio sources from deep…

We present the results of studying the accretion disk vs jet power for a large fraction of all the blazars detected by the Fermi Gamma-Ray Space Telescope. The disk power is inferred from the emission line luminosities obtained from…

High Energy Astrophysical Phenomena · Physics 2022-09-27 Garima Rajguru , Ritaban Chatterjee

We study a large sample of narrow-line radio galaxies (NLRGs) with extended radio structures. Using 1.4 GHz radio luminosities, $L_{1.4}$, narrow optical emission line luminosities, $L_{\oiii}$ and $L_{H_{\alpha}}$, as well as black hole…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Marek Sikora , Grażyna Stasińska , Dorota Kozieł-Wierzbowska , Greg M. Madejski , Natalia V. Asari

Aims. We use a sample of 83 core-dominated active galactic nuclei (AGN) selected from the MOJAVE (Monitoring of Jets in AGN with VLBA Experiments) radio-flux-limited sample and detected with the Fermi Large Area Telescope (LAT) to study the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 T. G. Arshakian , J. León-Tavares , M. Boettcher , J. Torrealba , V. H. Chavushyan , M. L. Lister , E. Ros , J. A. Zensus

We analyze the jet-disk coupling for different subsamples from a complete hard X-ray Seyfert sample to study the coupling indices and their relation to accretion rate. The results are: (1) the power-law coupling index ranges from nearly…

High Energy Astrophysical Phenomena · Physics 2021-09-21 Xiang Liu , Ning Chang , Zhenhua Han , Xin Wang

We present the space density evolution, from z=1.5 up to z=5.5, of the most massive (M$\geq10^9$M$_{\odot}$) black holes hosted in jetted Active Galactic Nuclei(AGNs). The analysis is based on a sample of 380 luminosity-selected…

The Fermi Gamma-ray Space Telescope with its main instrument on-board, the Large Area Telescope (LAT), opened a new era in the study of high-energy emission from Active Galactic Nuclei (AGN). When combined with contemporaneous ground- and…

High Energy Astrophysical Phenomena · Physics 2017-12-01 Filippo D'Ammando

To constrain models of the jet-disc connection, we explore Eddington ratios reported in Foschini (2011) and interpret them in relation to the values in Sikora et al. across the active galactic nuclei population from radio loud quasars,…

High Energy Astrophysical Phenomena · Physics 2013-07-31 David Garofalo

Jet origination is one of the most important questions of AGN, yet it stays obscure. In this work, we made use of information of emission lines, spectral energy distributions (SEDs), \textit{Fermi}-LAT $\gamma$-ray emission, construct a…

High Energy Astrophysical Phenomena · Physics 2022-02-02 Hubing Xiao , Zhihao OuYang , Lixia Zhang , Liping Fu , Shaohua Zhang , Xiangtao Zeng , Junhui Fan

Blazar subclasses ranging from flat-spectrum radio quasars (FSRQs) through low-frequency-peaked BL Lac objects (LBLs) to high-frequency-peaked BL Lac objects (HBLs) exhibit a sequence of increasing spectral hardness with decreasing…

Astrophysics · Physics 2009-11-06 M. Boettcher , C. D. Dermer

Three-dimensional simulations of relativistic jets are a useful tool to understand the evolution of jets and radio galaxies in detail. However, computationally demanding as they are, their use is limited to a relatively small number of…

Cosmology and Nongalactic Astrophysics · Physics 2026-01-14 Pau Beltrán-Palau , Manel Perucho , José María Martí

Understanding the evolution of accretion activity is fundamental to our understanding of how galaxies form and evolve over the history of the Universe. We analyse a complete sample of 27 radio galaxies which includes both high-excitation…

We present the general properties of the Active Galactic Nuclei (AGNs) and discuss the origin and structure of jets that are associated to a fraction of these objects. We then we address the problems of particle acceleration at highly…

Astrophysics · Physics 2010-12-13 S. Massaglia

We collect a large sample with a reliable redshift detected by the Fermi satellite after 10 years of data (4FGL-DR2), including blazars, $\gamma$-ray Narrow-line Seyfert 1 galaxies ($\gamma$NLS1s), and radio galaxies. The spectral energy…

High Energy Astrophysical Phenomena · Physics 2023-02-23 Chen Yongyun , Gu Qiusheng , Fan Junhui , Yu Xiaoling , Ding Nan , Xiong Dingrong , Guo Xiaotong
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