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Related papers: Microquasars in the GeV-TeV era

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The gamma-ray binaries LS 5039 and LS I +61 303 have been detected by Cerenkov telescopes at TeV energies, exhibiting periodic behavior correlated with the orbital period. These gamma-ray binary systems have also been recently detected by…

High Energy Astrophysical Phenomena · Physics 2010-08-04 Diego F. Torres

The launch of the Fermi gamma-ray space telescope and the imaging air Cerenkov telescopes H.E.S.S., MAGIC, and VERITAS have substantially transformed our knowledge of gamma-ray sources in the last decade. The extragalactic gamma-ray sky is…

High Energy Astrophysical Phenomena · Physics 2013-09-02 C. Pfrommer

Massive protostars have associated bipolar outflows with velocities of hundreds of km/s. Such outflows produce strong shocks when interact with the ambient medium leading to regions of non-thermal radio emission. Under certain conditions,…

High Energy Astrophysical Phenomena · Physics 2009-08-07 Gustavo E. Romero , Anabella T. Araudo , Valenti Bosch-Ramon , Josep M. Paredes

After initial claims and a long hiatus, it is now established that several binary stars emit high (0.1-100 GeV) and very high energy (>100 GeV) gamma rays. A new class has emerged called 'gamma-ray binaries', since most of their radiated…

High Energy Astrophysical Phenomena · Physics 2013-09-06 Guillaume Dubus

The detection of fast variations of the TeV (10^12 eV) gamma-ray flux, on time-scales of days, from the nearby radio galaxy M 87 is reported. These variations are ~10 times faster than that observed in any other waveband and imply a very…

Astrophysics · Physics 2008-11-26 HESS Collaboration , F. A. Aharonian

The development of techniques whereby gamma rays of energy 100 GeV and above can be studied from the ground, using indirect, but sensitive, techniques has opened up a new area of high energy photon astronomy. The most exciting result that…

Astrophysics · Physics 2009-11-10 D. Horan , T. C. Weekes

The impact of non-thermal processes on the spectral energy distributions of galaxies can be dramatic, but such processes are often neglected in considerations of their structure and evolution. Particle acceleration associated with high mass…

High Energy Astrophysical Phenomena · Physics 2015-06-04 S. Ohm , J. A. Hinton

Black holes (BH), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass BHs drive relativistic jets when accreting matter from their…

High Energy Astrophysical Phenomena · Physics 2026-01-01 The LHAASO Collaboration , Zhen Cao , Felix Aharonian , Yun-Xiang Bai , Yi-Wei Bao , Denis Bastieri , Xiao-Jun Bi , Yu-Jiang Bi , Wen-Yi Bian , Anatoly V Bukevich , Chengmiao Cai , Wen-Yu Cao , Zhe Cao , Jin Chang , Jin-Fan Chang , Aming Chen , En-Sheng Chen , Guohai Chen , Hua-Xi Chen , Liang Chen , Long Chen , Ming-Jun Chen , Ma-Li Chen , Qi-Hui Chen , Shi Chen , Su-Hong Chen , Song-Zhan Chen , Tian-Lu Chen , Xiao-Bin Chen , Xuejian Chen , Yang Chen , Ning Cheng , Yao-Dong Cheng , Ming Chung Chu , Ming-Yang Cui , Shu-Wang Cui , Xiao-Hong Cui , Yi-Dong Cui , Ben-Zhong Dai , Hong-Liang Dai , Zigao Dai , Danzeng Luobu , Yang-Xuan Diao , Xu-Qiang Dong , Kai-Kai Duan , Jun-Hui Fan , Yi-Zhong Fan , Jun Fang , Jian-Hua Fang , Kun Fang , Cun-feng Feng , Hua Feng , Li Feng , Shaohui Feng , Xiao-ting Feng , Yi Feng , You-liang Feng , Stefano Gabici , Bo Gao , Chuan-dong Gao , Qi Gao , Wei Gao , Wei-kang Gao , Maomao Ge , Ting-Ting Ge , Lisi Geng , Gwenael Giacinti , Guanghua Gong , Quanbu Gou , Min-Hao Gu , Fu-Lai Guo , Jing Guo , Xiao-Lei Guo , Yi-Qing Guo , Ying-Ying Guo , Yi-Ang Han , Otto A Hannuksela , Mariam Hasan , Hui-Hai He , Hao-Ning He , Jia-Yin He , Xinyu He , Yu He , Sergio Hernández-Cadena , Bo-Wen Hou , Chao Hou , Xian Hou , Hong-Bo Hu , Shi-Cong Hu , Chen Huang , Dai-Hui Huang , Jiajun Huang , Tian-Qi Huang , Wen-Jun Huang , Xing-Tao Huang , Xiao-Yuan Huang , Yong Huang , Yi-Yun Huang , Xiao-Lu Ji , Huan-Yu Jia , Kang Jia , Hou-Bing Jiang , Kun Jiang , Xiao-Wei Jiang , Ze-Jun Jiang , Min Jin , Samy Kaci , Ming-Ming Kang , Ivan Karpikov , Dmitry Khangulyan , Denis Kuleshov , Kirill Kurinov , Bing-Bing Li , Cheng Li , Cong Li , Dan Li , Fei Li , Haibo Li , Huicai Li , Jian Li , Jie Li , Kai Li , Long Li , Rong-Lan Li , Si-Da Li , Tian-Yang Li , Wen-Lian Li , Xiu-Rong Li , Xin Li , Yuan Li , Yizhuo Li , Zhe Li , Zhuo Li , En-Wei Liang , Yun-Feng Liang , Su-Jie Lin , Bing Liu , Cheng Liu , Dong Liu , Dang-Bo Liu , Hu Liu , Hai-Dong Liu , Jia Liu , Jia-Li Liu , Ji-Ren Liu , Mao-Yuan Liu , Ruo-Yu Liu , Si-Ming Liu , Wei Liu , X Liu , Yi Liu , Yu Liu , Yi-Nong Liu , Yu-Qing Lou , Qing Luo , Yu Luo , Hong-Kui Lv , Bo-Qiang Ma , Ling-Ling Ma , Xin-Hua Ma , Ji-Rong Mao , Zhen Min , Warit Mitthumsiri , Guo-Bin Mou , Hui-Jun Mu , Andrii Neronov , Kenny Chun Yu NG , Ming-Yang Ni , Lin Nie , Le-Jian Ou , Petchara Pattarakijwanich , Zhi-Yuan Pei , Jin-Can Qi , Meng-Yao Qi , Jia-Jun Qin , Ali Raza , Chong-Yang Ren , David Ruffolo , Alejandro Sáiz , Dmitri Semikoz , Lang Shao , Oleg Shchegolev , Yun-Zhi Shen , Xiang-Dong Sheng , Zhaodong Shi , Fu-Wen Shu , Hui-Chao Song , Yuri V Stenkin , Vladimir Stepanov , Yang Su , Dongxu Sun , Hao Sun , Qinning Sun , Xiaona Sun , Zhibin Sun , Nabeel Hussain Tabasam , Jumpei Takata , Pak Hin Thomas Tam , Hong-Bin Tan , Qingwen Tang , Ruiyi Tang , Zebo Tang , Wenwu Tian , Chaonan Tong , Li-Hong Wan , Chao Wang , Guangwei Wang , Hongguang Wang , Jiancheng Wang , Ke Wang , Kai Wang , Liping Wang , Lingyu Wang , Lu-Yao Wang , Ran Wang , Wei Wang , Xianggao Wang , Xin-Jian Wang , Xiang-Yu Wang , Yang Wang , Yu-Dong Wang , Zhong-Hai Wang , Zhong-Xiang Wang , Zheng Wang , Da-Ming Wei , Jun-Jie Wei , Yong-Jian Wei , Tao Wen , Shan-Shan Weng , Chao-Yong Wu , Han-Rong Wu , Qing-Wen Wu , Sha Wu , Xue-Feng Wu , Yu-Sheng Wu , Shao-qiang Xi , Jie Xia , Jun-Ji Xia , Guang-man Xiang , Di-xuan Xiao , Gang Xiao , Yu-liang Xin , Yi Xing , Ding-rong Xiong , Zeng Xiong , Dong-lian Xu , Reng-Feng Xu , Ren-Xin Xu , Wei-Li Xu , Liang Xue , Da-Hai Yan , Jing-Zhi Yan , Tian Yan , Chao-Wen Yang , Chu-Yuan Yang , Feng-Fan Yang , Li-Li Yang , Ming-Jie Yang , Rui-Zhi Yang , Wen-Xin Yang , Zihang Yang , Zhi-Guo Yao , Xuan-Ang Ye , Li-Qiao Yin , Na Yin , Xiao-Hao You , Zhi-Yong You , Yan-Hong Yu , Qiang Yuan , Hua Yue , Hou-Dun Zeng , Ting-Xuan Zeng , Wei Zeng , Xiangtao Zeng , Min Zha , Bin-Bin Zhang , Bing Theodore Zhang , Chao Zhang , Feng Zhang , Hong-Fei Zhang , Hai-Ming Zhang , Heng-Ying Zhang , Jian-Li Zhang , Li Zhang , Peng-Fei Zhang , Pei-Pei Zhang , Rui Zhang , Shao-Ru Zhang , Shou-Shan Zhang , Weiyan Zhang , Xiao Zhang , Xiao-Peng Zhang , Yi Zhang , Yong Zhang , Zhi-Peng Zhang , Jing Zhao , Lei Zhao , Li-Zhi Zhao , Shi-Ping Zhao , Xiao-Hong Zhao , Zihao Zhao , Fu Zheng , Wen-Juan Zhong , Bin Zhou , Hao Zhou , Jia-Neng Zhou , Meng Zhou , Ping Zhou , Rong Zhou , Xiao-Xi Zhou , Xun-Xiu Zhou , Ben-Yang Zhu , Cheng-Guang Zhu , Feng-Rong Zhu , Hui Zhu , Ke-Jun Zhu , Yuan-Chuan Zou , Xiong Zuo

In recent years, blazar surveys at radio and X-ray energies have greatly increased our understanding of this type of active galaxy. The combination of multi-wavelength data has shown that blazars follow a well defined sequence in terms of…

Astrophysics · Physics 2007-05-23 I. de la Calle Perez

A cluster of galaxies is a huge system bounded by gravitation, and cosmic rays are thought to be confined in the system, thus it should contain much non-thermal components. Many theories predict significant gamma-ray emission that could be…

High Energy Astrophysical Phenomena · Physics 2009-12-18 Masaki Mori

Microquasars, compact binary systems with an accreting stellar-mass black hole or neutron star, are promising candidates for high-energy particle acceleration. Recently, the LHAASO collaboration reported on the detection of $>100$ TeV…

High Energy Astrophysical Phenomena · Physics 2026-01-21 Jose Carpio , Ali Kheirandish , Bing Zhang

We study the gamma-ray emissions from an outer-magnetospheric potential gap around a rotating neutron star. Migratory electrons and positrons are accelerated by the electric field in the gap to radiate copious gamma-rays via curvature…

Astrophysics · Physics 2009-10-31 K. Hirotani

We investigate gamma-ray emission in the impulsive phase of solar flares and the detectability of non-thermal signatures from protostellar flares. Energetic solar flares emit high-energy gamma rays of GeV energies, but their production…

High Energy Astrophysical Phenomena · Physics 2023-03-08 Shigeo S. Kimura , Shinsuke Takasao , Kengo Tomida

Microquasars, the local siblings of extragalactic quasars, are binary systems comprising a compact object and a companion star. By accreting matter from their companions, microquasars launch powerful winds and jets, influencing the…

High Energy Astrophysical Phenomena · Physics 2020-08-25 Jian Li , Diego F. Torres , Ruo-Yu Liu , Matthew Kerr , Emma de Ona Wilhelmi , Yang Su

Microquasars are laboratories for the study of jets of relativistic particles produced by accretion onto a spinning black hole. Microquasars are near enough to allow detailed imaging of spatial features across the multiwavelength spectrum.…

The high-energy radiation from short period binaries containing a massive star with a compact relativistic companion was detected from radio to TeV gamma rays. We show here that PeV regime protons can be efficiently accelerated in the…

High Energy Astrophysical Phenomena · Physics 2021-11-01 A. M. Bykov , A. E. Petrov , M. E. Kalyashova , S. V. Troitsky

Recent ground based and space telescopes that detect high energy photons from a few up to hundreds of gigaelectron volts (GeV) have opened a new window on the universe. However, because of the relatively poor angular resolution of these…

High Energy Astrophysical Phenomena · Physics 2015-06-03 I. F. Mirabel

During last years a few massive binary systems have been detected in the TeV gamma-rays. This gamma-ray emission is clearly modulated with the orbital periods of these binaries suggesting its origin inside the binary system. In this paper…

Astrophysics · Physics 2008-06-27 W. Bednarek

We consider the neutron star (NS) of the magnetar type inside the massive binary system. We determine the conditions under which the matter from the stellar wind can penetrate the inner magnetosphere of the magnetar. At some distance from…

High Energy Astrophysical Phenomena · Physics 2015-05-13 W. Bednarek

Microquasars, X-ray binary systems that generate relativistic jets, were discovered in our Galaxy in the last decade of the XXth century. Their name indicates that they are manifestations of the same physics as quasars but on a completely…

Astrophysics · Physics 2009-11-11 M. M. Kaufman Bernado