English
Related papers

Related papers: M87 as a misaligned Synchrotron-Proton Blazar

200 papers

Several low-power kiloparsec-scale jets in nearby radio galaxies are known for their synchrotron radiation extending up to optical and X-ray photon energies. Here we comment on high-energy gamma-ray emission of one particular object of this…

Astrophysics · Physics 2009-11-10 L. Stawarz , A. Siemiginowska , M. Ostrowski , M. Sikora

Context. The radio galaxy IC310 in the Perseus cluster has recently been detected in the gamma-ray regime at GeV and TeV energies. The TeV emission shows time variability and an extraordinarily hard spectrum, even harder than the spectrum…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Matthias Kadler , Dorit Eisenacher , Eduardo Ros , Karl Mannheim , Dominik Elsässer , Uwe Bach

The spectra of BL Lac objects and Fanaroff-Riley I radio galaxies are commonly explained by the one-zone leptonic synchrotron self-Compton (SSC) model. Spectral modeling of correlated multiwavelength data gives the comoving magnetic field…

High Energy Astrophysical Phenomena · Physics 2012-03-27 Kohta Murase , Charles D. Dermer , Hajime Takami , Giulia Migliori

Non-blazar Active Galactic Nuclei (AGN) have emerged as a new gamma-ray emitting source class on the extragalactic sky and started to deepen our understanding of the physical processes and the nature of AGN in general. The detection of…

High Energy Astrophysical Phenomena · Physics 2017-07-10 Frank M. Rieger

(abridged) MGRO J2019+37 is an unidentified extended source of VHE gamma-rays originally reported by the Milagro Collaboration as the brightest TeV source in the Cygnus region. Its extended emission could be powered by either a single or…

The Local Group dwarf elliptical galaxy M32 hosts one of the nearest and most under-luminous super-massive black holes (SMBHs) ever known, offering a rare opportunity to study the physics of accreting SMBHs at the most quiescent state.…

Astrophysics of Galaxies · Physics 2020-05-13 Sijia Peng , Zhiyuan Li , Loránt O. Sjouwerman , Yang Yang , Fuguo Xie , Feng Yuan

We study the contribution of thermal and non-thermal processes to the inverse Compton emission of the radio galaxy M 87 by modelling its broad-band emission. Through this we aim to derive insight into where within the AGN the X-ray,…

High Energy Astrophysical Phenomena · Physics 2015-04-27 S. de Jong , V. Beckmann , S. Soldi , A. Tramacere , A. Gros

M87 is the first detected non-blazar extragalactic Tera-Electron-Volt (TeV) source with rapid variation and very flat spectrum in the TeV band. To explain the two-peaks in the spectral energy distribution (SED) of the nucleus of M87 which…

High Energy Astrophysical Phenomena · Physics 2012-02-13 Yu-Dong Cui , Ye-Fei Yuan , Yan-Rong Li , Jian-Min Wang

Blazars with redshifts z<0.1 are likely candidates for detection at energies in the range 300 GeV - 50 TeV with Cerenkov telescopes and scintillator arrays. We present gamma-ray flux predictions for a sample of 15 nearby flat-spectrum radio…

Astrophysics · Physics 2011-05-23 K. Mannheim , S. Westerhoff , H. Meyer , H. -H. Fink

Motivated by unification schemes of active galactic nuclei, we review evidence for the existence of a small-scale dust torus in M87, a Fanaroff-Riley Class I radio galaxy. Since there is no direct evidence of any thermal emission from its…

Astrophysics · Physics 2007-05-23 A. -C. Donea , R. J. Protheroe

The recent detection of TeV gamma-radiation from the direction of the Galactic Center within several arc-minutes around Sgr A* is the first model-independent evidence of existence of high energy particle accelerator(s) in the central 10 pc…

Astrophysics · Physics 2007-05-23 F. Aharonian , A. Neronov

We present the results of a multi-wavelength study of a population of X-ray bright ($\rm log(F_{0.2-12 \ keV})>-12.5$), non-$\gamma$-ray detected high and extreme high synchrotron peak (HSP, EHSP; $\rm log(\nu_{\rm peak,\ Hz})>16$) BL Lacs…

High Energy Astrophysical Phenomena · Physics 2026-04-29 Federica Sibani , Stefano Marchesi , Ettore Bronzini , Marco Ajello , Michele Doro , Lea Marcotulli , Elisa Prandini , Cristian Vignali

The possible origin of millisecond bursts from the giant elliptical galaxy M87 has been scrutinized since the earliest searches for extragalactic fast radio transients undertaken in the late 1970s. Motivated by rapid technological…

High Energy Astrophysical Phenomena · Physics 2021-10-13 Akshay Suresh , Shami Chatterjee , James M. Cordes , Fronefield Crawford

Non-blazar AGN have been recently established as a class of gamma-ray sources. M87, a nearby representative of this class, show fast TeV variability on timescales of a few days. We suggest a scenario of flare gamma-ray emission in…

High Energy Astrophysical Phenomena · Physics 2010-12-01 Maxim V. Barkov , Felix A. Aharonian , Valenti Bosch-Ramon

Several BL Lac objects are confirmed sources of variable and strongly Doppler-boosted TeV emission produced in the nuclear portions of their relativistic jets. It is more than probable, that also many of the FR I radio galaxies, believed to…

Astrophysics · Physics 2009-11-11 L. Stawarz , F. Aharonian , S. Wagner , M. Ostrowski

Spiral galaxies M31 and M33 are Fermi/LAT-detected gamma-ray sources. We model the broadband non-thermal (NT) emission of the central region of M31 (R < 5.5 kpc) and of the disk of M33 (R ~ 9 kpc). For either galaxy, we self-consistently…

High Energy Astrophysical Phenomena · Physics 2024-05-16 Massimo Persic , Yoel Rephaeli , Riccardo Rando

We present a multi-wavelength study of IC 1531 (z=0.02564), an extragalactic radio source associated with the $\gamma$-ray object 3FGL J0009.9-3206 and classified as a blazar of uncertain type in the Third Fermi Large Area Telescope AGN…

High Energy Astrophysical Phenomena · Physics 2018-10-17 T. Bassi , G. Migliori , P. Grandi , C. Vignali , M. A. Pérez-Torres , R. D. Baldi , E. Torresi , A. Siemiginowska , C. Stanghellini

Using observations carried out with the GMRT, we performed high-quality full-synthesis imaging at 610 MHz of the source G29.37+0.1, which is an as-yet-unclassified object linked to the TeV source HESS J1844-030. These data, combined with…

Astrophysics of Galaxies · Physics 2017-05-31 G. Castelletti , L. Supan , A. Petriella , E. Giacani , B. C. Joshi

The radio galaxy M87 has recently been found to be a rapidly variable TeV emitting source. We analyze the implications of the observed TeV characteristics and show that it proves challenging to account for them within conventional…

Astrophysics · Physics 2011-03-10 F. M. Rieger , F. A. Aharonian

We investigate the nature and classification of PMNJ1603-4904, a bright radio source close to the Galactic plane, which is associated with one of the brightest hard-spectrum gamma-ray sources detected by Fermi/LAT. It has previously been…