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We present preliminary results of our work on blazar unification. We assume that all blazars have a broad line region (BLR) and that the size of the BLR scales with the power of the source in a manner similar to that derived through…

Astrophysics · Physics 2007-05-23 Markos Georganopoulos , John G. Kirk , Apostolos Mastichiadis

We report radio imaging and monitoring observations in the frequency range 0.235 - 2.7 GHz during the flaring mode of PKS 2155-304, one of the brightest BL Lac objects. The high sensitivity GMRT observations not only reveal extended…

High Energy Astrophysical Phenomena · Physics 2016-10-19 M. Pandey-Pommier , S. Sirothia , P. Chadwick , J. -M. Martin , P. Colom , W. van Driel , F. Combes , P. Kharb , P-J. Crespeau , J. Richard , B. Guiderdoni

We have recently proposed a new simplified scenario where blazars are classified as flat-spectrum radio quasars (FSRQs) or BL Lacs according to the prescriptions of unified schemes, and to a varying combination of Doppler boosted radiation…

High Energy Astrophysical Phenomena · Physics 2015-06-15 P. Giommi , P. Padovani , G. Polenta

We use the third catalog of blazars detected by Fermi/LAT (3LAC) and gamma-ray Narrow-line Seyfert 1 Galaxies (gamma-NLSy1s) to study the blazar sequence and relationship between them. Our results are as follows: (i) There is a weak…

High Energy Astrophysical Phenomena · Physics 2021-03-03 Yongyun Chen , Qiusheng Gu , Junhui Fan , Hongtao Wang , Nan Ding , Xiaolin Yu , Xiaotong Guo , Dingrong Xiong , Shaojie Qin

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

A model is developed for the time dependent electromagnetic - radio to gamma-ray - emission of active galactic nuclei, specifically, the blazars, based on the acceleration and creation of leptons at a propagating discontinuity or {\it…

Astrophysics · Physics 2008-02-03 M. M. Romanova , R. V. E. Lovelace

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

In this paper, we use the quasi-simultaneous spectra of Fermi bright blazars and Fermi detected narrow line Seyfert 1 (NLS1) to study the blazar sequence and inverse Compton (IC) models. I. The synchrotron peak luminosities (L_{s})…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Liang Chen , J. M. Bai

We examine the long term (~10 years) gamma-ray variability of blazars observed by EGRET and Fermi and find that for six sources the average flux varied by more than an order of magnitude. For two of these sources (PKS 0208-512 and PKS…

Cosmology and Nongalactic Astrophysics · Physics 2013-03-26 Debbijoy Bhattacharya , Ranjeev Misra , A. R. Rao , P. Sreekumar

Compton scattering of external radiation by nonthermal particles in outflowing blazar jets is dominated by accretion-disk photons rather than scattered radiation to distances $\sim 0.01-0.1$ pc from the central engine for standard…

Astrophysics · Physics 2007-05-23 Charles D. Dermer , Reinhard Schlickeiser

Blazars, a subset of powerful active galactic nuclei, feature relativistic jets that shine in a broadband electromagnetic radiation, e. g. from radio to TeV emission. Here I present the results of the studies that explore gamma-ray and…

High Energy Astrophysical Phenomena · Physics 2022-10-18 Gopal Bhatta

We propose and test a fairly simple idea that could account for the blazar sequence: all jets are launched with similar energy per baryon, independently of their power. For instance, flat-spectrum radio quasars (FSRQs), the most powerful…

High Energy Astrophysical Phenomena · Physics 2021-01-13 Jesús M. Rueda-Becerril , Amanda O. Harrison , Dimitrios Giannios

We construct a large sample of gamma-ray blazars with low-frequency radio data using the recent released TGSS AD1 catalog at 150 MHz. The radio/gamma connections of blazars are compared from 143 GHz to 150 MHz. The radio flux density at all…

High Energy Astrophysical Phenomena · Physics 2018-12-26 Xu-Liang Fan , Qingwen Wu

Multiwavelength observations are essential to constrain physical parameters of the blazars observed by Fermi/LAT. Among the 187 AGN significantly detected in public INTEGRAL data above 20 keV by the imager IBIS/ISGRI, 20 blazars were…

High Energy Astrophysical Phenomena · Physics 2009-12-14 V. Beckmann , C. Ricci , S. Soldi

We compute the contribution of blazars (Flat Spectrum Radio Quasars and BL-Lacs) to the Fermi-LAT Extragalactic gamma-ray Background, assuming a gamma-ray luminosity function proportional to the luminosity function of radio galaxies and the…

High Energy Astrophysical Phenomena · Physics 2011-11-01 Massimo Cavadini , Ruben Salvaterra , Francesco Haardt

Recent detection of suborbital gamma-ray variability of Flat Spectrum Radio Quasar (FSRQ) 3C 279 by Fermi Large Area Telescope (LAT) is in severe conflict with established models of blazar emission. This paper presents the results of…

High Energy Astrophysical Phenomena · Physics 2017-12-15 Krzysztof Nalewajko

Multi-wavelength analyses of spectra of active galactic nuclei (AGNs) provide useful information on the physical processes in the accretion disk and jets of black holes. This, however, is limited to bright sources and may not represent the…

High Energy Astrophysical Phenomena · Physics 2021-06-09 Houdun Zeng , Vahé Petrosian , Tingfeng Yi

The Fermi Large Area Telescope (Fermi LAT) provides long term systematic monitoring observations of the gamma-ray emission from blazars. The variability properties and the correlation with other wavelength bands are important clues for the…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Stefan Larsson

We present the results of a multi-frequency, time-averaged analysis of blazars included in the Candidate Gamma-ray Blazar Survey catalog. Our sample consists of 324 $\gamma$-ray detected ($\gamma$-ray loud) and 191 non $\gamma$-ray detected…

High Energy Astrophysical Phenomena · Physics 2017-12-20 Vaidehi S. Paliya , L. Marcotulli , M. Ajello , M. Joshi , S. Sahayanathan , A. R. Rao , D. Hartmann
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