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Related papers: Highly Variable $\gamma$-Ray Emission of CTD 135 a…

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We present the results of a series of 3D special relativistic hydrodynamic simulations of a gamma-ray burst (GRB) jet in a massive circumstellar medium (CSM) surrounding the progenitor star. Our simulations reproduce the jet morphology…

High Energy Astrophysical Phenomena · Physics 2024-06-12 Akihiro Suzuki , Christopher M. Irwin , Keiichi Maeda

This Letter presents the first results from the observations of LSI +61 303 using Large Area Telescope data from the Fermi Gamma-Ray Space Telescope between 2008 August and 2009 March. Our results indicate variability that is consistent…

High Energy Astrophysical Phenomena · Physics 2019-08-13 A. A. Abdo

Most pulsars observed by the Fermi LAT have gamma-ray luminosities scaling with spindown power Edot as L_gamma (Edot x 10^33 erg/s)^{1/2}. However, there exist one detection and several upper limits an order of magnitude or more fainter…

High Energy Astrophysical Phenomena · Physics 2015-05-28 R. W. Romani , M. Kerr , H. A. Craig , S. Johnston , I. Cognard , D. A. Smith

In the framework of the TANAMI multi-wavelength and VLBI monitoring, we study the evolution of the parsec-scale radio emission in radio galaxies in the southern hemisphere and their relationship to the $\gamma$-ray properties. In this first…

The fast TeV variability of the blazars Mrk 501 and PKS 2155--304 implies a compact emitting region that moves with a bulk Lorentz factor of Gamma_{em}~100 toward the observer. The Lorentz factor is clearly in excess of the jet Lorentz…

High Energy Astrophysical Phenomena · Physics 2009-11-13 Dimitrios Giannios , Dmitri A. Uzdensky , Mitchell C. Begelman

Most of the radio-loud narrow-line Seyfert 1 (NLS1) galaxies resemble compact steep-spectrum sources. However, the extremely radio-loud ones show blazar-like characteristics, like flat radio spectra, compact radio cores, substantial…

Astrophysics of Galaxies · Physics 2018-07-18 K. É. Gabányi , A. Moór , S. Frey

We present the results of a program to monitor the structure of the radio emission in 42 $\gamma$-ray bright blazars (31 quasars and 11 BL Lac objects) with the VLBA at 43, 22, and occasionally 15 and 8.4 GHz, over the period from November…

The large-scale diffuse $\gamma-$ray flux observed by Fermi-LAT in the 1-100 GeV energy range, parameterized as $\propto E^{-\Gamma}$, has a spectral index $\Gamma$ that depends on the distance from the Galactic center. This feature, if…

High Energy Astrophysical Phenomena · Physics 2023-08-25 Vittoria Vecchiotti , Giulia Pagliaroli , Francesco Lorenzo Villante

We investigate the $\gamma$-ray and X-ray properties of the flat spectrum radio quasar (FSRQ) \4c50 at redshift $z= 1.517$. The {\it Fermi} Large Area Telescope (LAT) data indicate that this source was in an active state since 2013 July.…

High Energy Astrophysical Phenomena · Physics 2021-06-03 Jianeng Zhou , V. Jithesh , Chen Liang , Zhongxiang Wang

We present multi-wavelength monitoring results for the broad-line radio galaxy 3C 120 in the MeV/GeV, sub-millimeter, and 43 GHz bands over six years. Over the past two years, Fermi-LAT sporadically detected 3C 120 with high significance…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Y. T. Tanaka , A. Doi , Y. Inoue , C. C. Cheung , L. Stawarz , Y. Fukazawa , M. A. Gurwell , M. Tahara , J. Kataoka , R. Itoh

The diffuse Galactic gamma-ray emission is produced by cosmic rays (CRs) interacting with the interstellar gas and radiation field. Measurements by the Energetic Gamma-Ray Experiment Telescope (EGRET) instrument on the Compton Gamma-Ray…

High Energy Astrophysical Phenomena · Physics 2010-04-23 LAT Collaboration

Characteristic variability timescales in blazar gamma-ray light curves can provide insight into the physical processes responsible for the gamma-ray variability. The power spectral density (PSD) is capable of revealing such timescales,…

High Energy Astrophysical Phenomena · Physics 2019-11-06 James L. Ryan , Aneta Siemiginowska , Malgosia Sobolewska , Jonathan Grindlay

The Large Area Telescope (LAT) onboard the {\it Fermi} Gamma Ray Space Telescope has detected \gamma-ray emission from some Narrow Line Seyfert 1(NLSy1) galaxies. This indicates the presence of relativistic jets in these sources similar to…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Vaidehi S. Paliya , C. S. Stalin , Brijesh Kumar , Brajesh Kumar , V. K. Bhatt , S. B. Pandey , R. K. S. Yadav

Compact Symmetric Objects (CSOs) are a distinct category of jetted active galactic nuclei (AGN) whose optical variability characteristics have not been well investigated. We present here the results of our investigation on the optical flux…

Astrophysics of Galaxies · Physics 2025-05-07 Subhashree Swain , Vaidehi S. Paliya , D. J. Saikia , C. S. Stalin , Arya Venugopal , A. K. Bhavya , C. D. Ravikumar

We present an in-depth and systematic variability study of a sample of 20 powerful blazars, including 12 BL Lacs and 8 flat spectrum radio quasars, applying various analysis tools such as flux distribution, symmetry analysis, and time…

High Energy Astrophysical Phenomena · Physics 2020-03-18 Gopal Bhatta , Niraj Dhital

The Galactic high-mass X-ray binary and jet source (microquasar) LSI +61 303 has recently been detected at TeV gamma-ray energies by the MAGIC telescope. We have applied a time-dependent leptonic jet model to the broadband spectral energy…

Astrophysics · Physics 2011-02-11 Swati Gupta , Markus Boettcher

In this paper we report on the two-year-long Fermi-LAT observation of the peculiar blazar 4C +21.35 (PKS 1222+216). This source was in a quiescent state from the start of science operations of the Fermi Gamma-ray Space Telescope in 2008…

Hadron emission from supernova remnant (SNR)-molecular cloud (MC) association systems has been widely regarded as a probe of the shock-accelerated cosmic-ray protons. Here, we report on the detection of a {\gamma}-ray emission source, with…

High Energy Astrophysical Phenomena · Physics 2015-08-19 Bing Liu , Yang Chen , Xiao Zhang , Gao-Yuan Zhang , Yi Xing , Thomas G. Pannuti

We present a multi-wavelength study of four high redshift blazars, S5 0014+81 ($z=3.37$), CGRaBS J0225+1846 ($z=2.69$), BZQ J1430+4205 ($z=4.72$), and 3FGL J1656.2$-$3303 ($z=2.40$), using the quasi-simultaneous data from {\it Swift}, {\it…

High Energy Astrophysical Phenomena · Physics 2016-07-06 Vaidehi S. Paliya , M. L. Parker , A. C. Fabian , C. S. Stalin