Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433
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.S.S.) and found an energy-dependent shift in the apparent position of the gamma-ray emission from the parsec-scale jets. These...
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| Vydané v: | Science (American Association for the Advancement of Science) Ročník 383; číslo 6681; s. 402 |
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| Hlavní autori: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Médium: | Journal Article |
| Jazyk: | English |
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United States
26.01.2024
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| ISSN: | 1095-9203, 1095-9203 |
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| Abstract | 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.S.S.) and found an energy-dependent shift in the apparent position of the gamma-ray emission from the parsec-scale jets. These observations trace the energetic electron population and indicate that inverse Compton scattering is the emission mechanism of the gamma rays. Our modeling of the energy-dependent gamma-ray morphology constrains the location of particle acceleration and requires an abrupt deceleration of the jet flow. We infer the presence of shocks on either side of the binary system, at distances of 25 to 30 parsecs, and that self-collimation of the precessing jets forms the shocks, which then efficiently accelerate electrons. |
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| AbstractList | 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.S.S.) and found an energy-dependent shift in the apparent position of the gamma-ray emission from the parsec-scale jets. These observations trace the energetic electron population and indicate that inverse Compton scattering is the emission mechanism of the gamma rays. Our modeling of the energy-dependent gamma-ray morphology constrains the location of particle acceleration and requires an abrupt deceleration of the jet flow. We infer the presence of shocks on either side of the binary system, at distances of 25 to 30 parsecs, and that self-collimation of the precessing jets forms the shocks, which then efficiently accelerate electrons. 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.S.S.) and found an energy-dependent shift in the apparent position of the gamma-ray emission from the parsec-scale jets. These observations trace the energetic electron population and indicate that inverse Compton scattering is the emission mechanism of the gamma rays. Our modeling of the energy-dependent gamma-ray morphology constrains the location of particle acceleration and requires an abrupt deceleration of the jet flow. We infer the presence of shocks on either side of the binary system, at distances of 25 to 30 parsecs, and that self-collimation of the precessing jets forms the shocks, which then efficiently accelerate electrons.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.S.S.) and found an energy-dependent shift in the apparent position of the gamma-ray emission from the parsec-scale jets. These observations trace the energetic electron population and indicate that inverse Compton scattering is the emission mechanism of the gamma rays. Our modeling of the energy-dependent gamma-ray morphology constrains the location of particle acceleration and requires an abrupt deceleration of the jet flow. We infer the presence of shocks on either side of the binary system, at distances of 25 to 30 parsecs, and that self-collimation of the precessing jets forms the shocks, which then efficiently accelerate electrons. |
| Author | Aharonian, F Doroshenko, V Katarzyński, K Borowska, J Einecke, S Nakashima, K Kostunin, D Cerruti, M Jamrozy, M Montanari, A Glawion, D Holler, M Celic, J Hinton, J A Kluźniak, W Kosack, K Backes, M Ernenwein, J-P Klepser, S Martí-Devesa, G Burger-Scheidlin, C Casanova, S Gabici, S Leuschner, F Funk, S Batzofin, R Giavitto, G Brun, F Khatoon, R Mohrmann, L Lenain, J-P Dmytriiev, A Mbarubucyeye, J Damascene Hofmann, W Lypova, I Bi, B Mitchell, A Lohse, T Moulin, E Marx, R Murach, T Cotter, G Le Stum, S Bruno, B Ghafourizadeh, S Kasai, E Cecil, R Egberts, K Haerer, L Moderski, R Lang, R G Füßling, M Boisson, C Martins, V Barbosa Chandra, S Bernlöhr, K Leitl, F Mehta, A Böttcher, M Bouyahiaoui, M Marchegiani, P de Naurois, M Khélifi, B de Lavergne, M de Bony Bolmont, J Marandon, V Benkhali, F Ait Brown, A M Brose, R Komin, Nu Luashvili, A Jung-Richardt, I Caroff, S Fontaine, G Grolleron, G Filipovic, M Joshi, V Breuhaus, M Mackey, J Holch, T L Bulik, T Chibueze, O Horns, D Chand, T Glicenstein, J-F Djannati-Ataï, A Aschersleben, J Dai, S Chen, A Kundu, A Berge, D Jankowsky, F Ja |
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Marx fullname: Marx, R organization: Landessternwarte, Universität Heidelberg, Heidelberg D-69117, Germany – sequence: 92 givenname: A surname: Mehta fullname: Mehta, A organization: Deutsches Elektronen-Synchrotron, Zeuthen D-15738, Germany – sequence: 93 givenname: A surname: Mitchell fullname: Mitchell, A organization: Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen D-91058, Germany – sequence: 94 givenname: R surname: Moderski fullname: Moderski, R organization: Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw 00-716, Poland – sequence: 95 givenname: L surname: Mohrmann fullname: Mohrmann, L organization: Max-Planck-Institut für Kernphysik, Heidelberg D-69117, Germany – sequence: 96 givenname: A surname: Montanari fullname: Montanari, A organization: Landessternwarte, Universität Heidelberg, Heidelberg D-69117, Germany – sequence: 97 givenname: E surname: Moulin fullname: Moulin, E organization: Institute for Research on the Fundamental Laws of the Universe, Commissariat à l'énergie atomique et aux énergies alternatives, Université Paris-Saclay, Gif-sur-Yvette F-91191, France – sequence: 98 givenname: T surname: Murach fullname: Murach, T organization: Deutsches Elektronen-Synchrotron, Zeuthen D-15738, Germany – sequence: 99 givenname: K surname: Nakashima fullname: Nakashima, K organization: Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen D-91058, Germany – sequence: 100 givenname: M surname: de Naurois fullname: de Naurois, M organization: Laboratoire Leprince-Ringuet, École Polytechnique, Centre national de la recherche scientifique, Institut Polytechnique de Paris, Palaiseau F-91128, France |
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| Snippet | 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... |
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| Title | Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433 |
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