English
Related papers

Related papers: Hadronic X-ray Flares from Blazars

200 papers

We perform an unbiased search of the origin of the recently observed 28 events above ~30 TeV in the IceCube neutrino observatory, assuming that these are (apart from the atmospheric background) of astrophysical origin produced by…

High Energy Astrophysical Phenomena · Physics 2013-10-30 Walter Winter

The recent detection of TeV gamma-rays from the microquasar LS 5039 by HESS is one of the most exciting discoveries of observational gamma-ray astronomy in the very high energy regime. This result clearly demonstrates that X-ray binaries…

The hypothesis that AGN jets might be the sources of the ultra-high energy cosmic rays has originally motivated the venture of TeV gamma ray astronomy. Surprisingly, after the discovery of TeV emission from blazars the attention has shifted…

Astrophysics · Physics 2010-12-13 Jorg P. Rachen

Radio flares have been postulated to be associated with the production of astrophysical neutrinos. For example, TXS 0506+056 exhibits a 2-3 yr delay between the 2017 IceCube-170922A/$\gamma$-ray flare and a GHz radio maximum. We…

High Energy Astrophysical Phenomena · Physics 2026-04-02 S. I. Stathopoulos , C. Yuan , G. Vasilopoulos , F. Testagrossa , D. Karavola , M. Petropoulou , W. Winter

The IceCube report of a $\sim 3.5\sigma$ excess of $13\pm5$ neutrino events in the direction of the blazar TXS 05056+056 in 2014-2015 and the 2017 detection of a high-energy neutrino, IceCube-170922A, during a gamma-ray flare from the same…

TeV $\gamma$-ray detections in flaring states without activity in X-rays from blazars have attracted much attention due to the irregularity of these "orphan" flares. Although the synchrotron self-Compton model has been very successful in…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Nissim Fraija

Solar flares convert magnetic energy into thermal and non-thermal plasma energy, the latter implying particle acceleration of charged particles such as protons. Protons are injected out of the coronal acceleration region and can interact…

High Energy Astrophysical Phenomena · Physics 2021-05-28 R. Abbasi , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , C. Alispach , A. A. Alves , N. M. Amin , R. An , K. Andeen , T. Anderson , I. Ansseau , G. Anton , C. Argüelles , S. Axani , X. Bai , A. Balagopal V. , A. Barbano , S. W. Barwick , B. Bastian , V. Basu , V. Baum , S. Baur , R. Bay , J. J. Beatty , K. -H. Becker , J. Becker Tjus , C. Bellenghi , S. BenZvi , D. Berley , E. Bernardini , D. Z. Besson , G. Binder , D. Bindig , E. Blaufuss , S. Blot , J. Borowka , S. Böser , O. Botner , J. Böttcher , E. Bourbeau , J. Bourbeau , F. Bradascio , J. Braun , S. Bron , J. Brostean-Kaiser , S. Browne , A. Burgman , R. S. Busse , M. A. Campana , C. Chen , D. Chirkin , S. Choi , B. A. Clark , K. Clark , L. Classen , A. Coleman , G. H. Collin , J. M. Conrad , P. Coppin , P. Correa , D. F. Cowen , R. Cross , P. Dave , C. De Clercq , J. J. DeLaunay , H. Dembinski , K. Deoskar , S. De Ridder , A. Desai , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , S. Dharani , A. Diaz , J. C. Díaz-Vélez , H. Dujmovic , M. Dunkman , M. A. DuVernois , E. Dvorak , T. Ehrhardt , P. Eller , R. Engel , H. Erpenbeck , J. Evans , P. A. Evenson , S. Fahey , A. R. Fazely , S. Fiedlschuster , A. T. Fienberg , K. Filimonov , C. Finley , L. Fischer , D. Fox , A. Franckowiak , E. Friedman , A. Fritz , P. Fürst , T. K. Gaisser , J. Gallagher , E. Ganster , S. Garrappa , L. Gerhardt , A. Ghadimi , C. Glaser , T. Glauch , T. Glüsenkamp , A. Goldschmidt , J. G. Gonzalez , S. Goswami , D. Grant , T. Grégoire , Z. Griffith , S. Griswold , M. Gündüz , C. Günther , C. Haack , A. Hallgren , R. Halliday , L. Halve , F. Halzen , M. Ha Minh , K. Hanson , J. Hardin , A. A. Harnisch , A. Haungs , S. Hauser , D. Hebecker , K. Helbing , F. Henningsen , E. C. Hettinger , S. Hickford , J. Hignight , C. Hill , G. C. Hill , K. D. Hoffman , R. Hoffmann , T. Hoinka , B. Hokanson-Fasig , K. Hoshina , F. Huang , M. Huber , T. Huber , K. Hultqvist , M. Hünnefeld , R. Hussain , S. In , N. Iovine , A. Ishihara , M. Jansson , G. S. Japaridze , M. Jeong , B. J. P. Jones , R. Joppe , D. Kang , W. Kang , X. Kang , A. Kappes , D. Kappesser , T. Karg , M. Karl , A. Karle , U. Katz , M. Kauer , M. Kellermann , J. L. Kelley , A. Kheirandish , J. Kim , K. Kin , T. Kintscher , J. Kiryluk , S. R. Klein , R. Koirala , H. Kolanoski , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , P. Koundal , M. Kovacevich , M. Kowalski , K. Krings , G. Krückl , N. Kurahashi , A. Kyriacou , C. Lagunas Gualda , J. L. Lanfranchi , M. J. Larson , F. Lauber , J. P. Lazar , K. Leonard , A. Leszczyńska , Y. Li , Q. R. Liu , E. Lohfink , C. J. Lozano Mariscal , L. Lu , F. Lucarelli , A. Ludwig , W. Luszczak , Y. Lyu , W. Y. Ma , J. Madsen , K. B. M. Mahn , Y. Makino , S. Mancina , I. C. Mariş , R. Maruyama , K. Mase , F. McNally , K. Meagher , A. Medina , M. Meier , S. Meighen-Berger , J. Merz , J. Micallef , D. Mockler , G. Momenté , T. Montaruli , R. W. Moore , R. Morse , M. Moulai , R. Naab , R. Nagai , U. Naumann , J. Necker , L. V. Nguyen , H. Niederhausen , M. U. Nisa , S. C. Nowicki , D. R. Nygren , A. Obertacke Pollmann , M. Oehler , A. Olivas , E. O'Sullivan , H. Pandya , D. V. Pankova , N. Park , G. K. Parker , E. N. Paudel , P. Peiffer , C. Pérez de los Heros , S. Philippen , D. Pieloth , S. Pieper , A. Pizzuto , M. Plum , Y. Popovych , A. Porcelli , M. Prado Rodriguez , P. B. Price , B. Pries , G. T. Przybylski , C. Raab , A. Raissi , M. Rameez , K. Rawlins , I. C. Rea , A. Rehman , R. Reimann , G. Renzi , E. Resconi , S. Reusch , W. Rhode , M. Richman , B. Riedel , S. Robertson , G. Roellinghoff , M. Rongen , C. Rott , T. Ruhe , D. Ryckbosch , D. Rysewyk Cantu , I. Safa , S. E. Sanchez Herrera , A. Sandrock , J. Sandroos , M. Santander , S. Sarkar , S. Sarkar , K. Satalecka , M. Scharf , M. Schaufel , H. Schieler , P. Schlunder , T. Schmidt , A. Schneider , J. Schneider , F. G. Schröder , L. Schumacher , S. Sclafani , D. Seckel , S. Seunarine , A. Sharma , S. Shefali , M. Silva , B. Skrzypek , B. Smithers , R. Snihur , J. Soedingrekso , D. Soldin , G. M. Spiczak , C. Spiering , J. Stachurska , M. Stamatikos , T. Stanev , R. Stein , J. Stettner , A. Steuer , T. Stezelberger , R. G. Stokstad , T. Stuttard , G. W. Sullivan , I. Taboada , F. Tenholt , S. Ter-Antonyan , S. Tilav , F. Tischbein , K. Tollefson , L. Tomankova , C. Tönnis , S. Toscano , D. Tosi , A. Trettin , M. Tselengidou , C. F. Tung , A. Turcati , R. Turcotte , C. F. Turley , J. P. Twagirayezu , B. Ty , M. A. Unland Elorrieta , N. Valtonen-Mattila , J. Vandenbroucke , D. van Eijk , N. van Eijndhoven , D. Vannerom , J. van Santen , S. Verpoest , M. Vraeghe , C. Walck , A. Wallace , T. B. Watson , C. Weaver , A. Weindl , M. J. Weiss , J. Weldert , C. Wendt , J. Werthebach , M. Weyrauch , B. J. Whelan , N. Whitehorn , K. Wiebe , C. H. Wiebusch , D. R. Williams , M. Wolf , K. Woschnagg , G. Wrede , J. Wulff , X. W. Xu , Y. Xu , J. P. Yanez , S. Yoshida , T. Yuan , Z. Zhang

We present the dissection in space, time, and energy of the region around the IceCube-170922A neutrino alert. This study is motivated by: (1) the first association between a neutrino alert and a blazar in a flaring state, TXS 0506+056; (2)…

High Energy Astrophysical Phenomena · Physics 2018-07-13 P. Padovani , P. Giommi , E. Resconi , T. Glauch , B. Arsioli , N. Sahakyan , M. Huber

The discovery of high-energy astrophysical neutrinos by IceCube kicked off a new line of research to identify the electromagnetic counterparts producing these neutrinos. Among the extragalactic sources, active galactic nuclei (AGN), and in…

High Energy Astrophysical Phenomena · Physics 2019-02-13 C. Righi , F. Tavecchio , L. Pacciani

Bright blazars were found to be prominent neutrino sources, and a number of IceCube events were associated with them. Evaluating high-energy photon emission of such blazars is crucial for better understanding of the processes and regions…

High Energy Astrophysical Phenomena · Physics 2024-06-04 A. V. Plavin , R. A. Burenin , Y. Y. Kovalev , A. A. Lutovinov , A. A. Starobinsky , S. V. Troitsky , E. I. Zakharov

In this work, I present a qualitative discussion on the prospect of production of ultra-high photons in blazars. The sources are a subclass of active galactic nuclei which host supermassive black holes and fire relativistic jets into the…

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

High-energy neutrino and $\gamma$-ray emission has been observed from the Galactic plane, which may come from individual sources and/or diffuse cosmic rays. We evaluate the contribution of these two components through the multimessenger…

High Energy Astrophysical Phenomena · Physics 2023-10-30 Ke Fang , Kohta Murase

Galactic sites of acceleration of cosmic rays to energies of order 10^15 eV and higher, dubbed PeVatrons, reveal themselves by recently discovered gamma radiation of energies above 100 TeV. However, joint gamma-ray and neutrino production,…

We investigate the spectrum of photohadronically produced neutrinos at very high energies (VHE, >10^14 eV) in astrophysical sources whose physical properties are constrained by their variability, in particular jets in Active Galactic Nuclei…

Astrophysics · Physics 2009-10-30 Jorg P. Rachen , P. Meszaros

Recently the IceCube collaboration and 15 other collaborations reported the spatial and temporal coincidence between the neutrino event IceCube-170922A and the radio-TeV activity of the blazar TXS 0506+056. Their further analysis on 9.5…

High Energy Astrophysical Phenomena · Physics 2018-08-28 Yun-Feng Liang , Hao-Ning He , Neng-Hui Liao , Yu-Liang Xin , Qiang Yuan , Yi-Zhong Fan

The diffuse neutrino flux from FRI and BL Lac type galaxies generated from interactions of their own gamma radiation with the gas and dust at the sources is reported. This neutrino-production channel has not been studied in detail up to…

High Energy Astrophysical Phenomena · Physics 2013-09-30 J. C. Arteaga-Velazquez

While active galactic nuclei with relativistic jets have long been prime candidates for the origin of extragalactic cosmic rays and neutrinos, the BL Lac object TXS 0506+056 is the first astrophysical source observed to be associated with…

High Energy Astrophysical Phenomena · Physics 2018-11-28 M. Cerruti , A. Zech , C. Boisson , G. Emery , S. Inoue , J. -P. Lenain

With the coincident detection of a gamma-ray flare and a neutrino from the blazar TXS 0506+056, Active Galactic Nuclei (AGN) have been put into focus as possible sources of the diffuse neutrino flux. We present a space and time-resolved…

High Energy Astrophysical Phenomena · Physics 2020-06-24 Mario R. Hoerbe , Paul J. Morris , Garret Cotter , Julia Becker Tjus

A high-energy muon neutrino event, IceCube-170922A, was recently discovered in both spatial and temporal coincidence with a gamma-ray flare of the blazar TXS 0506+056. It has been shown, with standard one-zone models, that neutrinos can be…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Rui Xue , Ruo-Yu Liu , Maria Petropoulou , Foteini Oikonomou , Ze-Rui Wang , Kai Wang , Xiang-Yu Wang
‹ Prev 1 4 5 6 7 8 10 Next ›