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FältnamnIndikatorerMetadata
00013774naa a2202245 4500
001oai:DiVA.org:lnu-120926
003SwePub
008230526s2023 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-1209262 URI
024a https://doi.org/10.1051/0004-6361/2022454592 DOI
040 a (SwePub)lnu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Aharonian, F.u Dublin Inst Adv Studies, Ireland;Max Planck Inst Kernphys, Germany4 aut
2451 0a HESS J1809-193 :b A halo of escaped electrons around a pulsar wind nebula?
264 c 2023-03-01
264 1b EDP Sciences,c 2023
338 a electronic2 rdacarrier
520 a Context. HESS J1809-193 is an unassociated very-high-energy gamma-ray source located on the Galactic plane. While it has been connected to the nebula of the energetic pulsar PSR J1809-1917, supernova remnants and molecular clouds present in the vicinity also constitute possible associations. Recently, the detection of gamma-ray emission up to energies of similar to 100 TeV with the HAWC observatory has led to renewed interest in HESS J1809-193.Aims. We aim to understand the origin of the gamma-ray emission of HESS J1809-193.Methods. We analysed 93.2 h of data taken on HESS J1809-193 above 0.27 TeV with the High Energy Stereoscopic System (H.E.S.S.), using a multi-component, three-dimensional likelihood analysis. In addition, we provide a new analysis of 12.5 yr of Fermi-LAT data above 1 GeV within the region of HESS J1809-193. The obtained results are interpreted in a time-dependent modelling framework.Results. For the first time, we were able to resolve the emission detected with H.E.S.S. into two components: an extended component (modelled as an elongated Gaussian with a 1-sigma semi-major and semi-minor axis of similar to 0.62 degrees and similar to 0.35 degrees, respectively) that exhibits a spectral cutoff at similar to 13 TeV, and a compact component (modelled as a symmetric Gaussian with a 1-sigma radius of similar to 0.1 degrees) that is located close to PSR J1809-1917 and shows no clear spectral cutoff. The Fermi-LAT analysis also revealed extended gamma-ray emission, on scales similar to that of the extended H.E.S.S. component.Conclusions. Our modelling indicates that based on its spectrum and spatial extent, the extended H.E.S.S. component is likely caused by inverse Compton emission from old electrons that form a halo around the pulsar wind nebula. The compact component could be connected to either the pulsar wind nebula or the supernova remnant and molecular clouds. Due to its comparatively steep spectrum, modelling the Fermi-LAT emission together with the H.E.S.S. components is not straightforward.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a acceleration of particles
653 a radiation mechanisms
653 a non-thermal
653 a pulsars
653 a individual
653 a PSR J1809-1917
653 a gamma rays
653 a general
653 a Astroparticle Physics
653 a Astropartikelfysik
700a Ait Benkhali, F.u Heidelberg Univ, Germany4 aut
700a Aschersleben, J.u Univ Groningen, Netherlands4 aut
700a Ashkar, H.u Ecole Polytech, France4 aut
700a Backes, M.u Univ Namibia, Namibia;North West Univ, South Africa4 aut
700a Barbosa Martins, V.u DESY, Germany4 aut
700a Batzofin, R.u Univ Witwatersrand, South Africa4 aut
700a Becherini, Yvonneu Linnéuniversitetet,Institutionen för fysik och elektroteknik (IFE),Univ Paris, France4 aut0 (Swepub:lnu)yvbeaa
700a Berge, D.u DESY, Germany;Humboldt Univ, Germany4 aut
700a Boettcher, M.u North West Univ, South Africa4 aut
700a Boisson, C.u Univ Paris, France4 aut
700a Bolmont, J.u Sorbonne Univ, France4 aut
700a Borowska, J.u Humboldt Univ, Germany4 aut
700a Bouyahiaoui, M.u Max Planck Inst Kernphys, Germany4 aut
700a Bradascio, F.u Univ Paris Saclay, France4 aut
700a Breuhaus, M.u Max Planck Inst Kernphys, Germany4 aut
700a Brose, R.u Dublin Inst Adv Studies, Ireland4 aut
700a Brun, F.u Univ Paris Saclay, France4 aut
700a Bruno, B.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Bulik, T.u Univ Warsaw, Poland4 aut
700a Burger-Scheidlin, C.u Dublin Inst Adv Studies, Ireland4 aut
700a Bylund, Tomasu Linnéuniversitetet,Institutionen för fysik och elektroteknik (IFE)4 aut0 (Swepub:lnu)tobyab
700a Caroff, S.u Univ Savoie Mont Blanc, France4 aut
700a Casanova, S.u Inst Fizyki Jdrowej PAN, Poland4 aut
700a Celic, J.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Cerruti, M.u Univ Paris, France4 aut
700a Chambery, P.u Univ Bordeaux, France4 aut
700a Chand, T.u North West Univ, South Africa4 aut
700a Chen, A.u Univ Witwatersrand, South Africa4 aut
700a Chibueze, J.u North West Univ, South Africa4 aut
700a Chibueze, O.u North West Univ, South Africa4 aut
700a Damascene Mbarubucyeye, J.u DESY, Germany4 aut
700a Djannati-Atai, A.u Univ Paris, France4 aut
700a Dmytriiev, A.u North West Univ, South Africa4 aut
700a Einecke, S.u Univ Adelaide, Australia4 aut
700a Ernenwein, J. -p.u Aix Marseille Univ, France4 aut
700a Feijen, K.u Univ Adelaide, Australia4 aut
700a Filipovic, M.u Western Sydney Univ, Australia4 aut
700a Fontaine, G.u Ecole Polytech, France4 aut
700a Fuessling, M.u DESY, Germany4 aut
700a Funk, S.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Gabici, S.u Univ Paris, France4 aut
700a Gallant, Y. A.u Univ Montpellier, France4 aut
700a Ghafourizadeh, S.u Heidelberg Univ, Germany4 aut
700a Giavitto, G.u DESY, Germany4 aut
700a Giunti, L.u Univ Paris, France;Univ Paris Saclay, France4 aut
700a Glawion, D.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Goswami, P.u North West Univ, South Africa4 aut
700a Grolleron, G.u Sorbonne Univ, France4 aut
700a Grondin, M. -h.u Univ Bordeaux, France4 aut
700a Haerer, L.u Max Planck Inst Kernphys, Germany4 aut
700a Hinton, J. A.u Max Planck Inst Kernphys, Germany4 aut
700a Hofmann, W.u Max Planck Inst Kernphys, Germany4 aut
700a Holch, T. L.u DESY, Germany4 aut
700a Holler, M.u Leopold Franzens Univ Innsbruck, Austria4 aut
700a Horns, D.u Univ Hamburg, Germany4 aut
700a Huang, Zhiqiuu Max Planck Inst Kernphys, Germany4 aut
700a Jamrozy, M.u Uniwersytet Jagiellonski, Poland4 aut
700a Jankowsky, F.u Heidelberg Univ, Germany4 aut
700a Joshi, V.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Jung-Richardt, I.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Kasai, E.u Univ Namibia, Namibia4 aut
700a Katarzynski, K.u Nicolaus Copernicus Univ, Poland4 aut
700a Khelifi, B.u Univ Paris, France4 aut
700a Kluzniak, W.u Polish Acad Sci, Poland4 aut
700a Komin, Nu.u Univ Witwatersrand, South Africa4 aut
700a Kosack, K.u Univ Paris Saclay, France4 aut
700a Kostunin, D.u DESY, Germany4 aut
700a Lang, R. G.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Le Stum, S.u Aix Marseille Univ, France4 aut
700a Leitl, F.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Lemiere, A.u Univ Paris, France4 aut
700a Lemoine-Goumard, M.u Univ Bordeaux, France4 aut
700a Lenain, J. -p.u Sorbonne Univ, France4 aut
700a Leuschner, F.u Univ Tubingen, Germany4 aut
700a Lohse, T.u Humboldt Univ, Germany4 aut
700a Luashvili, A.u Univ Paris, France4 aut
700a Lypova, I.u Heidelberg Univ, Germany4 aut
700a Mackey, J.u Dublin Inst Adv Studies, Ireland4 aut
700a Malyshev, D.u Univ Tubingen, Germany4 aut
700a Marandon, V.u Max Planck Inst Kernphys, Germany4 aut
700a Marchegiani, P.u Univ Witwatersrand, South Africa4 aut
700a Marcowith, A.u Univ Montpellier, France4 aut
700a Marinos, P.u Univ Adelaide, Australia4 aut
700a Marti-Devesa, G.u Leopold Franzens Univ Innsbruck, Austria4 aut
700a Marx, R.u Heidelberg Univ, Germany4 aut
700a Mitchell, A.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Moderski, R.u Polish Acad Sci, Poland4 aut
700a Mohrmann, L.u Max Planck Inst Kernphys, Germany4 aut
700a Montanari, A.u Univ Paris Saclay, France4 aut
700a Moulin, E.u Univ Paris Saclay, France4 aut
700a Muller, J.u Ecole Polytech, France4 aut
700a Nakashima, K.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a de Naurois, M.u Ecole Polytech, France4 aut
700a Niemiec, J.u Inst Fizyki Jdrowej PAN, Poland4 aut
700a Priyana Noel, A.u Uniwersytet Jagiellonski, Poland4 aut
700a Ohm, S.u DESY, Germany4 aut
700a Olivera-Nieto, L.u Max Planck Inst Kernphys, Germany4 aut
700a de Ona Wilhelmi, E.u DESY, Germany4 aut
700a Ostrowski, M.u Uniwersytet Jagiellonski, Poland4 aut
700a Panny, S.u Leopold Franzens Univ Innsbruck, Austria4 aut
700a Panter, M.u Max Planck Inst Kernphys, Germany4 aut
700a Parsons, R. D.u Humboldt Univ, Germany4 aut
700a Prokhorov, D. A.u Univ Amsterdam, Netherlands4 aut
700a Puehlhofer, G.u Univ Tubingen, Germany4 aut
700a Punch, M.u Univ Paris, France4 aut
700a Quirrenbach, A.u Heidelberg Univ, Germany4 aut
700a Reichherzer, P.u Univ Paris Saclay, France4 aut
700a Reimer, A.u Leopold Franzens Univ Innsbruck, Austria4 aut
700a Reimer, O.u Leopold Franzens Univ Innsbruck, Austria4 aut
700a Renaud, M.u Univ Montpellier, France4 aut
700a Reville, B.u Max Planck Inst Kernphys, Germany4 aut
700a Rieger, F.u Max Planck Inst Kernphys, Germany4 aut
700a Rowell, G.u Univ Adelaide, Australia4 aut
700a Rudak, B.u Polish Acad Sci, Poland4 aut
700a Sahakian, V.u Yerevan Phys Inst, Armenia4 aut
700a Santangelo, A.u Univ Tubingen, Germany4 aut
700a Sasaki, M.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Schutte, H. M.u North West Univ, South Africa4 aut
700a Schwanke, U.u Humboldt Univ, Germany4 aut
700a Shapopi, J. N. S.u Univ Namibia, Namibia4 aut
700a Sol, H.u Univ Paris, France4 aut
700a Specovius, A.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Spencer, S.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Stawarz, L.u Uniwersytet Jagiellonski, Poland4 aut
700a Steenkamp, R.u Univ Namibia, Namibia4 aut
700a Steinmassl, S.u Max Planck Inst Kernphys, Germany4 aut
700a Sushch, I.u North West Univ, South Africa4 aut
700a Suzuki, H.u Konan Univ, Japan4 aut
700a Takahashi, T.u Univ Tokyo, Japan4 aut
700a Tanaka, T.u Konan Univ, Japan4 aut
700a Terrier, R.u Univ Paris, France4 aut
700a Thorpe-Morgan, C.u Univ Tubingen, Germany4 aut
700a Tsirou, M.u Max Planck Inst Kernphys, Germany4 aut
700a Tsuji, N.u RIKEN, Japan4 aut
700a Uchiyama, Y.u Rikkyo Univ, Japan4 aut
700a van Eldik, C.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Vecchi, M.u Univ Groningen, Netherlands4 aut
700a Veh, J.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Venter, C.u North West Univ, South Africa4 aut
700a Vink, J.u Univ Amsterdam, Netherlands4 aut
700a Wach, T.u Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Wagner, S. J.u Heidelberg Univ, Germany4 aut
700a White, R.u Max Planck Inst Kernphys, Germany4 aut
700a Wierzcholska, A.u Inst Fizyki Jdrowej PAN, Poland4 aut
700a Wong, Yu Wunu Friedrich Alexander Univ Erlangen Nurnberg, Germany4 aut
700a Zacharias, M.u Heidelberg Univ, Germany;North West Univ, South Africa4 aut
700a Zargaryan, D.u Dublin Inst Adv Studies, Ireland4 aut
700a Zdziarski, A. A.u Polish Acad Sci, Poland4 aut
700a Zech, A.u Univ Paris, France4 aut
700a Zouari, S.u Univ Paris, France4 aut
700a Zywucka, N.u North West Univ, South Africa4 aut
710a Dublin Inst Adv Studies, Ireland;Max Planck Inst Kernphys, Germanyb Heidelberg Univ, Germany4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 672q 672x 0004-6361x 1432-0746
856u https://doi.org/10.1051/0004-6361/202245459y Fulltext
856u https://lnu.diva-portal.org/smash/get/diva2:1759626/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-120926
8564 8u https://doi.org/10.1051/0004-6361/202245459

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Aharonian, F.
Ait Benkhali, F.
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Reichherzer, P.
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Reimer, O.
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Rieger, F.
Rowell, G.
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