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Related papers: Unifying All Blazars

200 papers

We present an analysis of the cross-correlation between optical brightness and polarization degree in different types of blazars. The aim is to identify objects with simultaneous and consistent changes in characteristics and to determine if…

In this work, we collected a sample of BL Lacs, FR I and FR II(G) radio galaxies with available core and extended emissions from published works to discuss the unified schemes and estimate the Doppler factor for BL Lacs. Wilcoxon rank-sum…

Astrophysics of Galaxies · Physics 2021-11-18 Xu-Hong Ye , Jun-Hui Fan

The long-term variability of the multiwavelength blazar emission can be interpreted in terms of orientation variations of a helical, inhomogeneous, non-thermally emitting jet, possibly caused by the orbital motion of the parent black hole…

Astrophysics · Physics 2009-11-10 L. Ostorero , M. Villata , C. M. Raiteri

We have considered all blazars observed in the X-ray band and for which the slope of the X-ray spectrum is available. We have collected 421 spectra of 268 blazars, including 12 archival unpublished ASCA spectra of 7 blazars whose analysisis…

Astrophysics · Physics 2009-11-06 D. Donato , G. Ghisellini , G. Tagliaferri , G. Fossati

The multi-wavelength spectral and temporal variability observed in blazars set tight constraints on current theoretical emission models. Here, we investigate the relativistic magnetic reconnection process as a source of blazar emission in…

High Energy Astrophysical Phenomena · Physics 2018-12-04 I. M. Christie , M. Petropoulou , L. Sironi , D. Giannios

Both leptonic and hadronic emission processes may contribute to blazar jet emission; which dominates in blazars's high energy emission component remains an open question. Some intermediate synchrotron peaked blazars transition from their…

High Energy Astrophysical Phenomena · Physics 2022-06-01 Abel L. Peirson , Ioannis Liodakis , Roger W. Romani

In the first of a series of papers investigating emission from blazar jets from radio to high-energy {\gamma}-rays, we revisit the class of models where the jet has a uniform conical ballistic structure. We argue that by using simple…

High Energy Astrophysical Phenomena · Physics 2012-12-13 William J. Potter , Garret Cotter

The concept of the evolutionary sequence of jetted active galactic nuclei (AGNs) has been challenged in the last few decades since AGN subclasses are considered to be different due to their viewing angle. In this paper, we collected a…

Astrophysics of Galaxies · Physics 2022-01-26 Evaristus U. Iyida , Christian I. Eze , Finbarr C. Odo

With their emission mainly coming from a relativistic jet pointing towards us, blazars are fundamental sources to study extragalactic jets and their central engines, consisting of supermassive black holes (SMBHs) fed by accretion discs.…

We examine whether Flat Spectrum Radio Quasars (FSRQs) and BL Lacertae objects (BL Lacs) can act as plausible astrophysical sources of diffuse ultra-high-energy cosmic rays (UHECRs). Using realistic luminosity-dependent density evolution…

High Energy Astrophysical Phenomena · Physics 2026-05-20 Swaraj Pratim Sarmah , Umananda Dev Goswami

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

Blazars are a rare class of active galactic nuclei (AGN) with relativistic jets pointing towards the observer. Jets are thought to be launched as Poynting-flux dominated outflows that accelerate to relativistic speeds at the expense of the…

High Energy Astrophysical Phenomena · Physics 2022-11-16 Maria Petropoulou , Filippos Psarras , Dimitrios Giannios

BL Lac objects are active nuclei, hosted in massive elliptical galaxies, the emission of which is dominated by a relativistic jet closely aligned with the line of sight. This implies the existence of a parent population of sources with a…

High Energy Astrophysical Phenomena · Physics 2016-11-26 Renato Falomo , Elena Pian , Aldo Treves

Blazars are a subclass of radio-loud active galactic nuclei (AGNs), where the jet is aligned close to the line of sight. Blazars emission is dominated by non-thermal processes, where Doppler boosted radiation originates from a relativistic…

High Energy Astrophysical Phenomena · Physics 2021-08-19 Jakub Juryšek , Vitalii Sliusar , Dimitri Moulin , Roland Walter

A time-dependent emission model for blazar jets, taking acceleration due to Fermi-I and Fermi-II processes for electrons and protons as well as all relevant radiative processes self-consistently into account, is presented. The presence of…

High Energy Astrophysical Phenomena · Physics 2014-12-10 Matthias Weidinger , Felix Spanier

The X-ray spectrum of extreme HBL type blazars is located in the synchrotron branch of the broadband spectral energy distribution (SED), at energies below the peak. A joint fit of the extrapolated X-ray spectra together with a host galaxy…

High Energy Astrophysical Phenomena · Physics 2020-06-10 Alicja Wierzcholska , Stefan Wagner

Our understanding of the unification of jetted AGN has evolved greatly as jet samples have increased in size. Here, based on the largest-ever sample of over 2000 well-sampled jet spectral energy distributions, we examine the synchrotron…

Astrophysics of Galaxies · Physics 2021-05-12 Mary Keenan , Eileen T. Meyer , Markos Georganopoulos , Karthik Reddy , Omar J. French

We reevaluate 610 sources classified as Flat-spectrum radio quasars (FSRQs) in the 5th edition of the Roma-BZCAT. Optical spectra from SDSS DR16 confirm broad emission lines within $0.11 \leq z \leq 5.28$. To assess their blazar-like…

High Energy Astrophysical Phenomena · Physics 2026-05-26 Jonhatan U. Guerrero-González , Vahram Chavushyan , Víctor M. Patiño-Álvarez

BL Lac objects are the best candidates to study the jet properties since their spectral energy distributions (SEDs) are less contaminated by the emission from the accretion disk and external Compton processes. We compile the broadband SEDs…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Jin Zhang , En-Wei Liang , Shuang-Nan Zhang , Jin-Ming Bai

We present polarization images of 9 radio-loud (RL) quasars from the VLA B-array at 6 GHz. These quasars belong to the Palomar-Green (PG) "blazar" sample comprising 16 RL quasars and 8 BL Lac objects. Extensive polarization is detected in…

Astrophysics of Galaxies · Physics 2022-12-28 Janhavi Baghel , P. Kharb , Silpa S. , Luis C. Ho , C. M. Harrison