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Related papers: Revisiting the Blazar Main Sequence

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Statistical analyses are invaluable methods used to understand intrinsic emission processes and the unification of extragalactic radio sources. In this paper, we collected radio, X-ray and {\gamma}-ray data of blazars from the Fermi-LAT and…

High Energy Astrophysical Phenomena · Physics 2021-12-08 E. U. Iyida , I. O. Eya , F. C. Odo

The studies and constraints on the emission region are crucial to the blazar radiation mechanism. Yet the previous works mainly focus on individual sources. In this work, we make use of the largest and the latest spectral energy…

High Energy Astrophysical Phenomena · Physics 2023-07-17 Junhui Fan , Hubing Xiao , Wenxin Yang , Lixia Zhang , Anton A. Strigachev , Rumen S. Bachev , Jianghe Yang

Active galactic nuclei (AGNs) can power relativistic jets, which are called blazars when pointed close to our line of sight. Depending on the presence or absence of emission lines in their optical spectra, blazars are categorized into flat…

High Energy Astrophysical Phenomena · Physics 2024-04-23 Garima Rajguru , L. Marcotulli , M. Ajello , A. Tramacere

We present statistical analyses of a large homogenous data sample of Fermi-detected blazars thoroughly studied in order to reassess the relationship between flat-spectrum radio quasars (FSRQs) and subclasses of BL Lacertae objects (BL Lacs)…

High Energy Astrophysical Phenomena · Physics 2021-08-18 E. U. Iyida , F. C. Odo , A. E. Chukwude , A. A. Ubachukwu

We have not identified for sure what is the mechanism launching, accelerating and collimating relativistic jets. The two most likely possibilities are the gravitational energy of the accreting matter or the rotational energy of a spinning…

High Energy Astrophysical Phenomena · Physics 2018-09-21 Gabriele Ghisellini

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

The empirical relations in the black hole-accretion disk-relativistic jet system and physical processes behind these relations are still poorly understood, partly because they operate close to the black hole within the central light year.…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Tigran G. Arshakian , Vahram Chavushyan

We investigate the evolution of spectral energy distribution (SED) and underlying electron energy distribution (EED) by modeling the nearly simultaneous broadband spectra of selected bright 4FGL blazars, in the context of a combined cooling…

High Energy Astrophysical Phenomena · Physics 2025-09-04 Muhammad S. Anjum , Shu-Jin Hou , Liang Chen , Zhigang Li , Minfeng Gu

We fit the spectral energy distributions (SEDs) of members of a large sample of Fermi 2LAC blazars to synchrotron and inverse Compton (IC) models. Our main results are as follows. (i) As suggested by previous works, the correlation between…

High Energy Astrophysical Phenomena · Physics 2016-10-12 R. Xue , D. Luo , L. M. Du , Z. R. Wang , Z. H. Xie , T. F. Yi , D. R. Xiong , Y. B. Xu , W. G. Liu , X. L. Yu

The origin of jet launching mainly comes from two mechanisms: the BZ mechanism and the BP mechanism. However, it is in debate which one is dominating in blazars. In this work, we used a sample of 937 Fermi blazars to study the jet formation…

High Energy Astrophysical Phenomena · Physics 2024-11-19 Shangchun Xie , Zhihao Ouyang , Jingyu Wu , Hubing Xiao , Shaohua Zhang , Yongyun Chen , Zhijian Luo , Junhui Fan

The spectral properties of blazars seem to follow a phenomenological sequence according to the source luminosity. By inferring the source physical parameters through (necessarily) modeling the blazar spectra, we have previously proposed…

Astrophysics · Physics 2009-11-07 G. Ghisellini , A. Celotti , L. Costamante

The past 20 years have seen phenomenal progress in our understanding of BL Lac objects. They form part of the blazar class, which are radio-loud AGN whose relativistic jets are aligned along our line of sight. Several critical milestones…

Astrophysics · Physics 2007-05-23 C. Megan Urry

It is believed that jets emerging from blazars (Flat Spectrum Radio Quasars (FSRQs) and BL Lacs) are almost aligned to the line-of-sight. BL Lacs usually exhibit lower luminosity and harder power law spectra at gamma-ray energies than…

High Energy Astrophysical Phenomena · Physics 2013-02-15 Banibrata Mukhopadhyay

We revisit the so called "blazar sequence", which connects the observed bolometric luminosity to the shape of the spectral energy distribution (SED) of blazars. We propose that the power of the jet and the SED of its emission are linked to…

Astrophysics · Physics 2009-11-13 G. Ghisellini , F. Tavecchio

Blazars are a sub-class of quasars with Doppler boosted jets oriented close to the line of sight, and thus efficient probes of supermassive black hole growth and their environment, especially at high redshifts. Here we report on Very Long…

The limits on the mass of the black hole in 23 BL Lac objects are obtained from their luminosities of the broad emission line H\beta on the assumption that broad emission lines are emitted from clouds ionized by the radiation of the…

Astrophysics · Physics 2009-11-07 Xinwu Cao

With their rapid, violent variability and broad featureless continuum emission, blazars have puzzled astronomers for over two decades. Today blazars represent the only extragalactic objects detected in high-energy gamma-rays. Their spectral…

Astrophysics · Physics 2009-10-31 Eric S. Perlman

We study the general physical properties of Fermi blazars using the Fermi fourth source catalog data (4FGL-DR2). The quasi-simultaneous multiwavelength data of Fermi blazar are fitted by using the one-zone leptonic model to obtain some…

High Energy Astrophysical Phenomena · Physics 2023-07-03 Yongyun Chen , Qiusheng Gu , Junhui Fan , Xiaoling Yu , Xiaogu Zhong , Hongyu Liu , Nan Ding , Dingrong Xiong , Xiaotong Guo

General relativistic magnetohydrodynamic (GRMHD) simulations have been instrumental in our understanding of high energy astrophysical phenomena over the past two decades. Their robustness and modularity make them a great tool for…

High Energy Astrophysical Phenomena · Physics 2025-02-07 Mayank Pathak , Banibrata Mukhopadhyay

Flat Spectrum Radio Quasars (FSRQs) and BL Lac objects detected in the first three months of the Fermi survey neatly separate in the gamma-ray spectral index vs gamma-ray luminosity plane. BL Lac objects are less luminous and have harder…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 G. Ghisellini , L. Maraschi , F. Tavecchio