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Ultra-high-energy gamma-ray bubble around microquasar V4641 Sgr.
Nature
October 2024
Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai, China.
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 recent extension measurement of the spatial morphology of a microquasar, SS 433, to TeV gamma rays localizes the acceleration of electrons at shocks in the jet far from the black hole.
View Article and Find Full Text PDFAcceleration and transport of relativistic electrons in the jets of the microquasar SS 433.
Science
January 2024
Centre for Space Research, North-West University, Potchefstroom 2520, South Africa.
SS 433 is a microquasar, a stellar binary system that launches collimated relativistic jets. We observed SS 433 in gamma rays using the High Energy Stereoscopic System (H.E.
View Article and Find Full Text PDFSubsecond periodic radio oscillations in a microquasar.
Nature
September 2023
Department of Astronomy, School of Physics and Technology, Wuhan University, Wuhan, People's Republic of China.
Powerful relativistic jets are one of the ubiquitous features of accreting black holes in all scales. GRS 1915 + 105 is a well-known fast-spinning black-hole X-ray binary with a relativistic jet, termed a 'microquasar', as indicated by its superluminal motion of radio emission. It has exhibited persistent X-ray activity over the last 30 years, with quasiperiodic oscillations of approximately 1-10 Hz (refs.
View Article and Find Full Text PDFPublisher Correction: Very-high-energy particle acceleration powered by the jets of the microquasar SS 433.
Nature
December 2018
Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA.
In this Letter, owing to a production error, the penultimate version of the PDF was published. The HTML version was always correct. The PDF has been corrected online.
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