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Related papers: Gamma Rays from Compact Objects

200 papers

Thanks to the Fermi gamma-ray satellite and the current Imaging Atmospheric Cherenkov Telescopes, radio galaxies have arisen as a new class of high- and very-high energy emitters. The favourable orientation of their jets makes radio…

High Energy Astrophysical Phenomena · Physics 2020-04-08 Eleonora Torresi

Gamma-ray astronomy provides a direct window into the most violent, dynamic processes in the Universe. MeV gamma-ray astronomy in particular allows us to directly observe the process of chemical enrichment of the interstellar medium (ISM)…

High Energy Astrophysical Phenomena · Physics 2019-05-07 Fiona H. Panther

Studying the propagation of gamma rays on cosmological distances encompasses a variety of scientific fields, focusing on diffuse radiation fields such as the extragalactic background light, on the probe of the magnetism of the Universe on…

Cosmology and Nongalactic Astrophysics · Physics 2013-10-14 Jonathan Biteau

One of the main purposes in $\gamma$-ray astronomy is linked to the origin of Galactic cosmic rays. Unlike cosmic rays, $\gamma$ rays can be used to probe their production sites in the Galaxy and to find which type of astrophysical sources…

High Energy Astrophysical Phenomena · Physics 2024-12-18 J. Devin

The last decade has been dense with new developments in the search for the sources of Galactic cosmic rays. Some of these developments have confirmed the tight connection between cosmic rays and supernovae in our Galaxy, through the…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Pasquale Blasi

Gamma-ray studies are an essential tool in our search for the origin of cosmic rays. Instruments like the Fermi-LAT, H.E.S.S., MAGIC and VERITAS have revolutionized our understanding of the high energy Universe. This paper describes the…

High Energy Astrophysical Phenomena · Physics 2012-04-23 Stefan Funk

This white paper briefly summarizes the importance of the study of relativistic cosmic rays, both as a constituent of our Universe, and through their impact on stellar and galactic evolution. The focus is on what can be learned over the…

High Energy Astrophysical Phenomena · Physics 2021-06-16 A. Araudo , G. Morlino , B. Olmi , F. Acero , I. Agudo , R. Adam , R. Alves Batista , E. Amato , E. O. Anguner , L. A. Antonelli , Y. Ascasibar , C. Balazs , J. Becker Tjus , C. Bigongiari , E. Bissaldi , J. Bolmont , C. Boisson , P. Bordas , Ž. Bošnjak , A. M. Brown , M. Burton , N. Bucciantini , F. Cangemi , P. Caraveo , M. Cardillo , S. Caroff , S. Casanova , S. Chaty , M. Chernyakova , J. G. Coelho , F. Conte , G. Cotter , S. Crestan , A. D'Aì , E. M. de Gouveia Dal Pino , C. Delgado , D. della Volpe , D. de Martino , A. Djannati-Ataï , R. C. Dos Anjos , V. Dwarkadas , G. Emery , E. Fedorova , M. D. Filipovic , O. Fornieri , G. Galanti , D. Gasparrini , G. Ghirlanda , A. Giuliani , P. Goldoni , J. Granot , D. Grasso , E. de Oña Wilhelmi , B. Khélifi , M. Heller , D. Horan , B. Hnatyk , R. Hnatyk , S. Inoue , M. Jamrozy , N. Komin , A. Lamastra , N. La Palombara , J. -P. Lenain , I. Liodakis , S. Lombardi , F. Longo , A. Lòpez-Oramas , M. Lòpez-Moya , F. Lucarelli , P. L. Luque-Escamilla , P. Majumdar , A. Marcowith , J. Martì , M. Martinez , D. Mazin , S. Menchiari , L. Mohrmann , T. Montaruli , A. Morselli , C. G. Mundell , T. Murach , A. Nagai , A. Nayerhoda , J. Niemiec , M. Nikolajuk , R. A. Ong , J. M. Paredes , G. Pareschi , M. Pohl , G. Pühlhofer , M. Punch , O. Reimer , M. Ribò , F. Rieger , G. Rodriguez , G. Rowell , P. Romano , M. Roncadelli , G. Romeo , B. Rudak , F. Salesa Greus , F. G. Saturni , U. Sawangwit , F. Schüssler , O. Sergijenko , H. Sol , A. Stamerra , T. Stolarczyk , G. Tagliaferri , F. Tavecchio , V. Testa , L. Tibaldo , A. Viana , S. Vercellone , S. Ventura , J. Vink , S. Vorobiov , V. Vitale , I. Sadeh , P. Sharma , R. C. Shellard , T. Suomijärvi , A. Wierzcholska

The Atmospheric Cherenkov Imaging Technique has opened up the gamma-ray spectrumfrom 100 GeV to 50 TeV to astrophysical exploration. The development of the technique is described as are the basic principles underlying its use. The current…

Astrophysics · Physics 2007-05-23 Trevor C. Weekes

Transient and variable phenomena in astrophysical sources are of particular importance to understand the underlying gamma-ray emission processes. In the very-high energy gamma-ray domain, transient and variable sources are related to…

Instrumentation and Methods for Astrophysics · Physics 2020-02-26 F. Brun , Q. Piel , M. de Naurois , S. Bernhard

This paper summarizes the status of very high-energy (VHE) astronomy, as of early 2003. It concentrates on observations made by gamma-ray telescopes operating at energies above 10 GeV. This field is an exciting one to be working in, with a…

Astrophysics · Physics 2007-05-23 Rene A. Ong

Gamma-ray line observations provide a versatile tool for studies of nucleosynthesis processes and supernova physics. In particular, the observation of radioactive species in the interstellar medium probes recent nucleosynthesis activity on…

Astrophysics · Physics 2009-12-30 Jurgen Knodlseder

Clusters of galaxies and the large scale filaments that connect neighboring clusters are expected to be sites of acceleration of charged particles and sources of non-thermal radiation from radio frequencies to gamma rays. Gamma rays are…

Astrophysics · Physics 2009-11-13 Pasquale Blasi , Stefano Gabici , Gianfranco Brunetti

The field of ground-based gamma ray astronomy has enjoyed rapid growth in recent years. As an increasing number of sources are detected at TeV energies, the field has matured and become a viable branch of modern astronomy. Lying at the…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Wei Cui

The discovery of non-thermal X-ray emission from the jets of some X-ray binaries, and especially the discovery of GeV-TeV gamma-rays in some of them, provide a clear evidence of very efficient acceleration of particles to multi-TeV energies…

High Energy Astrophysical Phenomena · Physics 2010-01-26 J. M. Paredes , V. Zabalza

Very-high-energy (>100 GeV) gamma-ray astronomy is emerging as an important discipline in both high energy astrophysics and astro-particle physics. This field is currently dominated by Imaging Atmospheric-Cherenkov Telescopes (IACTs) and…

Astrophysics · Physics 2010-01-15 Jim Hinton

Compact relativistic jets in active galactic nuclei offer an effective tool for investigating the physics of nuclear regions in galaxies. The emission properties, dynamics, and evolution of jets in AGN are closely connected to the…

Astrophysics · Physics 2008-11-26 Andrei Lobanov

Very recently, the Tibet-AS$\gamma$ collaboration reported the detection of $\gamma$ rays from the galactic disk in the energy range of 100 TeV -- 1 PeV. Remarkably, many of these $\gamma$ rays were observed apart from known very high…

High Energy Astrophysical Phenomena · Physics 2021-04-08 Timur Dzhatdoev

Gamma-ray measurements from GeV to PeV energies have provided us with a wealth of information on diffuse emission and sources in the Universe lately. With improved spatial and temporal resolutions together with real-time multimessenger…

High Energy Astrophysical Phenomena · Physics 2025-04-02 Julia Becker Tjus , Julien Dörner , Leander Schlegel , Wolfgang Rhode

As the highest-energy photons, gamma rays have an inherent interest to astrophysicists and particle physicists studying high-energy, nonthermal processes. Gamma-ray telescopes complement those at other wavelengths, especially radio,…

Astrophysics · Physics 2009-11-10 David J. Thompson

In this paper I briefly review recent progress in the field of ground-based gamma ray astrophysics.

Astrophysics · Physics 2007-05-23 Wei Cui