Resolving acceleration to very high energies along the jet of Centaurus A

Abdalla H.; Adam R.; Aharonian F.; Benkhali F. Ait; Anguner E. O.; Arakawa M.; Arcaro C.; Armand C.; Ashkar H.; Backes M.; Barbosa Martins V.; Barnard M.; Becherini Y.; Berge D.; Bernloehr K.; Blackwell R.; Bottcher M.; Boisson C.; Bolmont J.; Bonnefoy S.; Bregeon J.; Breuhaus M.; Brun F.; Brun P.; Bryan M.; Buechele M.; Bulik T.; Bylund T.; Capasso M.; Caroff S.; Carosi A.; Casanova S.; Cerruti M.; Chand T.; Chandra S.; Chen A.; Colafrancesco S.; Curylo M.; Davids I. D.; Deil C.; Devin J.; DeWilt P.; Dirson L.; Djannati-Atai A.; Dmytriiev A.; Donath A.; Doroshenko V.; Drury L. OC.; Dyks J.; Egberts K.; Emery G.; Ernenwein J. -P.; Eschbach S.; Feijen K.; Fegan S.; Fiasson A.; Fontaine G.; Funk S.; Fuessling M.; Gabici S.; Gallant Y. A.; Gate F.; Giavitto G.; Glawion D.; Glicenstein J. F.; Gottschall D.; Grondin M. -H.; Hahn J.; Haupt M.; Heinzelmann G.; Henri G.; Hermann G.; Hinton J. A.; Hofmann W.; Hoischen C.; Holch T. L.; Holler M.; Horns D.; Huber D.; Iwasaki H.; Jamrozy M.; Jankowsky D.; Jankowsky F.; Jardin-Blicq A.; Jung-Richardt I.; Kastendieck M. A.; Katarzynski K.; Katsuragawa M.; Katz U.; Khangulyan D.; Khelifi B.; King J.; Klepser S.; Kluzniak W.; Komin N.; Kosack K.; Kostunin D.; Kraus M.; Lamanna G.; Lau J.; Lemiere A.; Lemoine-Goumard M.; Lenain J. -P.; Leser E.; Levy C.; Lohse T.; Lypova I.; Mackey J.; Majumdar J.; Malyshev D.; Marandon V.; Marcowith A.; Mares A.; Mariaud C.; Marti-Devesa G.; Marx R.; Maurin G.; Meintjes P. J.; Mitchell A. M. W.; Moderski R.; Mohamed M.; Mohrmann L.; Moore C.; Moulin E.; Muller J.; Murach T.; Nakashima S.; de Naurois M.; Ndiyavala H.; Niederwanger F.; Niemiec J.; Oakes L.; OBrien P.; Odaka H.; Ohm S.; de Ona Wilhelmi E.; Ostrowski M.; Oya I.; Panter M.; Parsons R. D.; Perennes C.; Petrucci P. -O.; Peyaud B.; Piel Q.; Pita S.; Poireau V.; Priyana Noel A.; Prokhorov D. A.; Prokoph H.; Puehlhofer G.; Punch M.; Quirrenbach A.; Raab S.; Rauth R.; Reimer A.; Reimer O.; Remy Q.; Renaud M.; Rieger F.; Rinchiuso L.; Romoli C.; Rowell G.; Rudak B.; Ruiz-Velasco E.; Sahakian V.; Saito S.; Sanchez D. A.; Santangelo A.; Sasaki M.; Schlickeiser R.; Schussler F.; Schulz A.; Schutte H. M.; Schwanke U.; Schwemmer S.; Seglar-Arroyo M.; Senniappan M.; Seyffert A. S.; Shafi N.; Shiningayamwe K.; Simoni R.; Sinha A.; Sol H.; Specovius A.; Spir-Jacob M.; Stawarz L.; Steenkamp R.; Stegmann C.; Steppa C.; Takahashi T.; Tavernier T.; Taylor A. M.; Terrier R.; Tiziani D.; Tluczykont M.; Trichard C.; Tsirou M.; Tsuji N.; Tuffs R.; Uchiyama Y.; van der Walt D. J.; van Eldik C.; van Rensburg C.; van Soelen B.; Vasileiadis G.; Veh J.; Venter C.; Vincent P.; Vink J.; Voisin F.; Voelk H. J.; Vuillaume T.; Wadiasingh Z.; Wagner S. J.; White R.; Wierzcholska A.; Yang R.; Yoneda H.; Zacharias M.; Zanin R.; Zdziarski A. A.; Zech A.; Ziegler A.; Zorn J.; Zywucka N.

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Resolving acceleration to very high energies along the jet of Centaurus A

机译：解决沿着滨海射流的加速度到非常高的能量a

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The nearby radio galaxy Centaurus A belongs to a class of active galaxies that are luminous at radio wavelengths. Most show collimated relativistic outflows known as jets, which extend over hundreds of thousands of parsecs for the most powerful sources. Accretion of matter onto the central supermassive black hole is believed to fuel these jets and power their emission(1). Synchrotron radiation from relativistic electrons causes the radio emission, and it has been suggested that the X-ray emission from Centaurus A also originates in electron synchrotron processes(2-4). Another possible explanation is inverse Compton scattering with cosmic microwave background (CMB) soft photons(5-7). Synchrotron radiation needs ultrarelativistic electrons (about 50 teraelectronvolts) and, given their short cooling times, requires some continuous re-acceleration mechanism(8). Inverse Compton scattering, on the other hand, does not require very energetic electrons, but the jets must stay highly relativistic on large scales (exceeding 1 megaparsec). Some recent evidence disfavours inverse Compton-CMB models(9-12), although other work seems to be compatible with them(13,14). In principle, the detection of extended gamma-ray emission, which directly probes the presence of ultrarelativistic electrons, could distinguish between these options. At gigaelectronvolt energies there is also an unusual spectral hardening(15,16)in Centaurus A that has not yet been explained. Here we report observations of Centaurus A at teraelectronvolt energies that resolve its large-scale jet. We interpret the data as evidence for the acceleration of ultrarelativistic electrons in the jet, and favour the synchrotron explanation for the X-rays. Given that this jet is not exceptional in terms of power, length or speed, it is possible that ultrarelativistic electrons are commonplace in the large-scale jets of radio-loud active galaxies.Observations of the radio galaxy Centaurus A at teraelectronvolt energies resolve its large-scale jet and favour electron synchrotron processes as the source of its X-ray emission.

机译：附近的无线电星座中心A属于一类在无线电波长的发光的活动星系。大多数显示准直相对主义的outflows称为喷射，这延长了最强大的资源的数十万个Parsecs。据信物质上的物质吸收，以燃料燃料，并为其发射（1）。来自相对论电子的同步辐射导致无线电发射，并提出了来自Civeraurus A的X射线发射也源于电子同步rotron方法（2-4）。另一种可能的解释是用宇宙微波背景（CMB）软光子（5-7）的逆符合康普顿散射。同步辐射需要超弧形的电子（约50个TERECOLTONVOLT），并且鉴于它们的冷却时间短，需要一些连续的再加速机制（8）。另一方面，逆康顿散射不需要非常精力充沛的电子，但喷气机必须在大尺度上保持高度相对论（超过1兆夸克）。一些最近的证据是反向康普顿-CMB模型（9-12），尽管其他工作似乎与他们兼容（13,14）。原则上，检测延长伽马射线发射，其直接探测紫外线电子的存在，可以区分这些选择。在GigaelectronVolt Energies，在尚未解释的中间人A中也存在一个不寻常的光谱硬化（15,16）。在这里，我们在TeraElectronVolt Energies中报告了Centaurus A的观察结果，可以解决其大规模喷射。我们将数据解释为射流加速超微征主义电子的证据，并有利于X射线的同步释放。鉴于该喷气机在功率，长度或速度方面不是出色的，可以在无线电活动星系的大规模喷气机中是普遍的普遍存在的无线电活跃的星系。在TeraElectronvolt Energies的无线电星系中心A的远程停泊状态分辨其大-scale jet并有利于电子同步加工作为其X射线发射的源。

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《Nature》 |2020年第7812期|356-359|共4页
作者
Abdalla H.; Adam R.; Aharonian F.; Benkhali F. Ait; Anguner E. O.; Arakawa M.; Arcaro C.; Armand C.; Ashkar H.; Backes M.; Barbosa Martins V.; Barnard M.; Becherini Y.; Berge D.; Bernloehr K.; Blackwell R.; Bottcher M.; Boisson C.; Bolmont J.; Bonnefoy S.; Bregeon J.; Breuhaus M.; Brun F.; Brun P.; Bryan M.; Buechele M.; Bulik T.; Bylund T.; Capasso M.; Caroff S.; Carosi A.; Casanova S.; Cerruti M.; Chand T.; Chandra S.; Chen A.; Colafrancesco S.; Curylo M.; Davids I. D.; Deil C.; Devin J.; DeWilt P.; Dirson L.; Djannati-Atai A.; Dmytriiev A.; Donath A.; Doroshenko V.; Drury L. OC.; Dyks J.; Egberts K.; Emery G.; Ernenwein J. -P.; Eschbach S.; Feijen K.; Fegan S.; Fiasson A.; Fontaine G.; Funk S.; Fuessling M.; Gabici S.; Gallant Y. A.; Gate F.; Giavitto G.; Glawion D.; Glicenstein J. F.; Gottschall D.; Grondin M. -H.; Hahn J.; Haupt M.; Heinzelmann G.; Henri G.; Hermann G.; Hinton J. A.; Hofmann W.; Hoischen C.; Holch T. L.; Holler M.; Horns D.; Huber D.; Iwasaki H.; Jamrozy M.; Jankowsky D.; Jankowsky F.; Jardin-Blicq A.; Jung-Richardt I.; Kastendieck M. A.; Katarzynski K.; Katsuragawa M.; Katz U.; Khangulyan D.; Khelifi B.; King J.; Klepser S.; Kluzniak W.; Komin N.; Kosack K.; Kostunin D.; Kraus M.; Lamanna G.; Lau J.; Lemiere A.; Lemoine-Goumard M.; Lenain J. -P.; Leser E.; Levy C.; Lohse T.; Lypova I.; Mackey J.; Majumdar J.; Malyshev D.; Marandon V.; Marcowith A.; Mares A.; Mariaud C.; Marti-Devesa G.; Marx R.; Maurin G.; Meintjes P. J.; Mitchell A. M. W.; Moderski R.; Mohamed M.; Mohrmann L.; Moore C.; Moulin E.; Muller J.; Murach T.; Nakashima S.; de Naurois M.; Ndiyavala H.; Niederwanger F.; Niemiec J.; Oakes L.; OBrien P.; Odaka H.; Ohm S.; de Ona Wilhelmi E.; Ostrowski M.; Oya I.; Panter M.; Parsons R. D.; Perennes C.; Petrucci P. -O.; Peyaud B.; Piel Q.; Pita S.; Poireau V.; Priyana Noel A.; Prokhorov D. A.; Prokoph H.; Puehlhofer G.; Punch M.; Quirrenbach A.; Raab S.; Rauth R.; Reimer A.; Reimer O.; Remy Q.; Renaud M.; Rieger F.; Rinchiuso L.; Romoli C.; Rowell G.; Rudak B.; Ruiz-Velasco E.; Sahakian V.; Saito S.; Sanchez D. A.; Santangelo A.; Sasaki M.; Schlickeiser R.; Schussler F.; Schulz A.; Schutte H. M.; Schwanke U.; Schwemmer S.; Seglar-Arroyo M.; Senniappan M.; Seyffert A. S.; Shafi N.; Shiningayamwe K.; Simoni R.; Sinha A.; Sol H.; Specovius A.; Spir-Jacob M.; Stawarz L.; Steenkamp R.; Stegmann C.; Steppa C.; Takahashi T.; Tavernier T.; Taylor A. M.; Terrier R.; Tiziani D.; Tluczykont M.; Trichard C.; Tsirou M.; Tsuji N.; Tuffs R.; Uchiyama Y.; van der Walt D. J.; van Eldik C.; van Rensburg C.; van Soelen B.; Vasileiadis G.; Veh J.; Venter C.; Vincent P.; Vink J.; Voisin F.; Voelk H. J.; Vuillaume T.; Wadiasingh Z.; Wagner S. J.; White R.; Wierzcholska A.; Yang R.; Yoneda H.; Zacharias M.; Zanin R.; Zdziarski A. A.; Zech A.; Ziegler A.; Zorn J.; Zywucka N.;
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North West Univ Ctr Space Res Potchefstroom South Africa;

CNRS Ecole Polytech Lab Leprince Ringuet Inst Polytech Paris IN2P3 UMR 7638 Palaiseau France|Univ Hamburg Inst Expt Phys Hamburg Germany;

Max Planck Inst Kernphys Heidelberg Germany|Dublin Inst Adv Studies Dublin Ireland|RAU High Energy Astrophys Lab Yerevan Armenia;

Max Planck Inst Kernphys Heidelberg Germany;

Aix Marseille Univ CNRS IN2P3 CPPM Marseille France;

Rikkyo Univ Dept Phys Tokyo Japan;

North West Univ Ctr Space Res Potchefstroom South Africa;

Univ Savoie Mt Blanc Univ Grenoble Alpes Lab Annecy Phys Particules CNRS LAPP Annecy France;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

North West Univ Ctr Space Res Potchefstroom South Africa|Univ Namibia Dept Phys Windhoek Namibia;

DESY Zeuthen Germany;

North West Univ Ctr Space Res Potchefstroom South Africa;

Linnaeus Univ Dept Phys & Elect Engn Vaxjo Sweden;

DESY Zeuthen Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Adelaide Sch Phys Sci Adelaide SA Australia;

North West Univ Ctr Space Res Potchefstroom South Africa;

Univ Paris Diderot PSL Res Univ Observ Paris LUTH CNRS Meudon France;

Sorbonne Univ Univ Paris Diderot Lab Phys Nucl & Hautes Energies CNRS IN2P3 LPNHE Sorbonne Paris Cite Paris France;

DESY Zeuthen Germany;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

Univ Amsterdam Anton Pannekoek Inst Astron GRAPPA Amsterdam Netherlands;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Univ Warsaw Astron Observ Warsaw Poland;

Linnaeus Univ Dept Phys & Elect Engn Vaxjo Sweden;

Univ Tubingen Inst Astron & Astrophys Tubingen Germany;

Sorbonne Univ Univ Paris Diderot Lab Phys Nucl & Hautes Energies CNRS IN2P3 LPNHE Sorbonne Paris Cite Paris France;

Univ Savoie Mt Blanc Univ Grenoble Alpes Lab Annecy Phys Particules CNRS LAPP Annecy France;

Max Planck Inst Kernphys Heidelberg Germany|Inst Fizyki Jadrowej PAN Krakow Poland;

Sorbonne Univ Univ Paris Diderot Lab Phys Nucl & Hautes Energies CNRS IN2P3 LPNHE Sorbonne Paris Cite Paris France|Univ Barcelona IEEC UB Inst Ciencies Cosmos ICC UB Barcelona Spain;

North West Univ Ctr Space Res Potchefstroom South Africa;

North West Univ Ctr Space Res Potchefstroom South Africa;

Univ Witwatersrand Sch Phys Johannesburg South Africa;

Univ Witwatersrand Sch Phys Johannesburg South Africa|Univ Hamburg Inst Expt Phys Hamburg Germany;

Univ Warsaw Astron Observ Warsaw Poland;

Univ Namibia Dept Phys Windhoek Namibia;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Bordeaux Ctr Etud Nucl Bordeaux Gradignan CNRS IN2P3 Gradignan France;

Univ Adelaide Sch Phys Sci Adelaide SA Australia;

Univ Hamburg Inst Expt Phys Hamburg Germany;

Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Univ Paris Diderot PSL Res Univ Observ Paris LUTH CNRS Meudon France;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Tubingen Inst Astron & Astrophys Tubingen Germany;

Dublin Inst Adv Studies Dublin Ireland;

Polish Acad Sci Nicolaus Copernicus Astron Ctr Warsaw Poland;

Univ Potsdam Inst Phys & Astron Potsdam Germany;

Sorbonne Univ Univ Paris Diderot Lab Phys Nucl & Hautes Energies CNRS IN2P3 LPNHE Sorbonne Paris Cite Paris France;

Aix Marseille Univ CNRS IN2P3 CPPM Marseille France;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Univ Adelaide Sch Phys Sci Adelaide SA Australia;

CNRS Ecole Polytech Lab Leprince Ringuet Inst Polytech Paris IN2P3 UMR 7638 Palaiseau France;

Aix Marseille Univ CNRS IN2P3 CPPM Marseille France;

CNRS Ecole Polytech Lab Leprince Ringuet Inst Polytech Paris IN2P3 UMR 7638 Palaiseau France;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

DESY Zeuthen Germany;

Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Univ Savoie Mt Blanc Univ Grenoble Alpes Lab Annecy Phys Particules CNRS LAPP Annecy France;

DESY Zeuthen Germany;

Heidelberg Univ Landessternwarte Heidelberg Germany;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

Univ Tubingen Inst Astron & Astrophys Tubingen Germany;

Univ Bordeaux Ctr Etud Nucl Bordeaux Gradignan CNRS IN2P3 Gradignan France;

Max Planck Inst Kernphys Heidelberg Germany;

DESY Zeuthen Germany;

Univ Hamburg Inst Expt Phys Hamburg Germany;

Univ Grenoble Alpes CNRS IPAG Grenoble France;

Max Planck Inst Kernphys Heidelberg Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Potsdam Inst Phys & Astron Potsdam Germany;

Humboldt Univ Inst Phys Berlin Germany;

Leopold Franzens Univ Innsbruck Inst Astro & Teilchenphys Innsbruck Austria;

Univ Hamburg Inst Expt Phys Hamburg Germany;

Leopold Franzens Univ Innsbruck Inst Astro & Teilchenphys Innsbruck Austria;

Rikkyo Univ Dept Phys Tokyo Japan;

Uniwersytet Jagiellonski Obserwatorium Astron Krakow Poland;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Heidelberg Univ Landessternwarte Heidelberg Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Univ Hamburg Inst Expt Phys Hamburg Germany;

Nicolaus Copernicus Univ Fac Phys Astron & Informat Ctr Astron Torun Poland;

Univ Tokyo Inst Adv Study UTIAS Kavli Inst Phys & Math Universe WPI Kashiwa Chiba Japan;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Rikkyo Univ Dept Phys Tokyo Japan;

Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Heidelberg Univ Landessternwarte Heidelberg Germany;

DESY Zeuthen Germany;

Polish Acad Sci Nicolaus Copernicus Astron Ctr Warsaw Poland;

Univ Witwatersrand Sch Phys Johannesburg South Africa;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

DESY Zeuthen Germany;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Univ Savoie Mt Blanc Univ Grenoble Alpes Lab Annecy Phys Particules CNRS LAPP Annecy France;

Univ Adelaide Sch Phys Sci Adelaide SA Australia;

Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Univ Bordeaux Ctr Etud Nucl Bordeaux Gradignan CNRS IN2P3 Gradignan France;

Sorbonne Univ Univ Paris Diderot Lab Phys Nucl & Hautes Energies CNRS IN2P3 LPNHE Sorbonne Paris Cite Paris France;

DESY Zeuthen Germany|Univ Potsdam Inst Phys & Astron Potsdam Germany;

Sorbonne Univ Univ Paris Diderot Lab Phys Nucl & Hautes Energies CNRS IN2P3 LPNHE Sorbonne Paris Cite Paris France;

Humboldt Univ Inst Phys Berlin Germany;

DESY Zeuthen Germany;

Dublin Inst Adv Studies Dublin Ireland;

DESY Zeuthen Germany;

Univ Tubingen Inst Astron & Astrophys Tubingen Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Univ Bordeaux Ctr Etud Nucl Bordeaux Gradignan CNRS IN2P3 Gradignan France;

CNRS Ecole Polytech Lab Leprince Ringuet Inst Polytech Paris IN2P3 UMR 7638 Palaiseau France;

Leopold Franzens Univ Innsbruck Inst Astro & Teilchenphys Innsbruck Austria;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Savoie Mt Blanc Univ Grenoble Alpes Lab Annecy Phys Particules CNRS LAPP Annecy France;

Univ Free State Dept Phys Bloemfontein South Africa;

Max Planck Inst Kernphys Heidelberg Germany|Univ Zurich Inst Phys Zurich Switzerland;

Polish Acad Sci Nicolaus Copernicus Astron Ctr Warsaw Poland;

Heidelberg Univ Landessternwarte Heidelberg Germany;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Univ Leicester Dept Phys & Astron Leicester LE1 7RH Leics England;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

CNRS Ecole Polytech Lab Leprince Ringuet Inst Polytech Paris IN2P3 UMR 7638 Palaiseau France;

DESY Zeuthen Germany;

RIKEN 2-1 Hirosawa Wako Saitama Japan;

CNRS Ecole Polytech Lab Leprince Ringuet Inst Polytech Paris IN2P3 UMR 7638 Palaiseau France;

North West Univ Ctr Space Res Potchefstroom South Africa;

Leopold Franzens Univ Innsbruck Inst Astro & Teilchenphys Innsbruck Austria;

Inst Fizyki Jadrowej PAN Krakow Poland;

Humboldt Univ Inst Phys Berlin Germany;

Univ Leicester Dept Phys & Astron Leicester LE1 7RH Leics England;

Univ Tokyo Dept Phys Tokyo Japan;

DESY Zeuthen Germany;

DESY Zeuthen Germany;

Uniwersytet Jagiellonski Obserwatorium Astron Krakow Poland;

DESY Zeuthen Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Sorbonne Univ Univ Paris Diderot Lab Phys Nucl & Hautes Energies CNRS IN2P3 LPNHE Sorbonne Paris Cite Paris France;

Univ Grenoble Alpes CNRS IPAG Grenoble France;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

Aix Marseille Univ CNRS IN2P3 CPPM Marseille France;

Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Univ Savoie Mt Blanc Univ Grenoble Alpes Lab Annecy Phys Particules CNRS LAPP Annecy France;

Uniwersytet Jagiellonski Obserwatorium Astron Krakow Poland;

Univ Witwatersrand Sch Phys Johannesburg South Africa;

DESY Zeuthen Germany;

Univ Tubingen Inst Astron & Astrophys Tubingen Germany;

Linnaeus Univ Dept Phys & Elect Engn Vaxjo Sweden|Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Heidelberg Univ Landessternwarte Heidelberg Germany;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Leopold Franzens Univ Innsbruck Inst Astro & Teilchenphys Innsbruck Austria;

Leopold Franzens Univ Innsbruck Inst Astro & Teilchenphys Innsbruck Austria;

Leopold Franzens Univ Innsbruck Inst Astro & Teilchenphys Innsbruck Austria;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Adelaide Sch Phys Sci Adelaide SA Australia;

Polish Acad Sci Nicolaus Copernicus Astron Ctr Warsaw Poland;

Max Planck Inst Kernphys Heidelberg Germany;

Yerevan Phys Inst Yerevan Armenia;

Rikkyo Univ Dept Phys Tokyo Japan;

Univ Savoie Mt Blanc Univ Grenoble Alpes Lab Annecy Phys Particules CNRS LAPP Annecy France;

Univ Tubingen Inst Astron & Astrophys Tubingen Germany;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Ruhr Univ Bochum Inst Theoret Phys Lehrstuhl Weltraum & Astrophys 4 Bochum Germany;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

DESY Zeuthen Germany;

North West Univ Ctr Space Res Potchefstroom South Africa;

Humboldt Univ Inst Phys Berlin Germany;

Heidelberg Univ Landessternwarte Heidelberg Germany;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

Linnaeus Univ Dept Phys & Elect Engn Vaxjo Sweden;

North West Univ Ctr Space Res Potchefstroom South Africa;

Univ Witwatersrand Sch Phys Johannesburg South Africa;

Univ Namibia Dept Phys Windhoek Namibia;

Univ Amsterdam Anton Pannekoek Inst Astron GRAPPA Amsterdam Netherlands;

Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Univ Paris Diderot PSL Res Univ Observ Paris LUTH CNRS Meudon France;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Uniwersytet Jagiellonski Obserwatorium Astron Krakow Poland;

Univ Namibia Dept Phys Windhoek Namibia;

DESY Zeuthen Germany|Univ Potsdam Inst Phys & Astron Potsdam Germany;

Univ Potsdam Inst Phys & Astron Potsdam Germany;

Univ Tokyo Inst Adv Study UTIAS Kavli Inst Phys & Math Universe WPI Kashiwa Chiba Japan;

Univ Paris Saclay CEA IRFU Gif Sur Yvette France;

DESY Zeuthen Germany;

Univ Paris Diderot Observ Paris AstroParticule & Cosmol APC CNRS IN2P3 CEA Irfu Sorbonne Paris Cite Paris France;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Univ Hamburg Inst Expt Phys Hamburg Germany;

CNRS Ecole Polytech Lab Leprince Ringuet Inst Polytech Paris IN2P3 UMR 7638 Palaiseau France;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Rikkyo Univ Dept Phys Tokyo Japan;

Max Planck Inst Kernphys Heidelberg Germany;

Rikkyo Univ Dept Phys Tokyo Japan;

North West Univ Ctr Space Res Potchefstroom South Africa;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

North West Univ Ctr Space Res Potchefstroom South Africa;

Univ Free State Dept Phys Bloemfontein South Africa;

Univ Montpellier Lab Univers & Particules Montpellier CNRS IN2P3 CC 72 Montpellier France;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

North West Univ Ctr Space Res Potchefstroom South Africa;

Sorbonne Univ Univ Paris Diderot Lab Phys Nucl & Hautes Energies CNRS IN2P3 LPNHE Sorbonne Paris Cite Paris France;

Univ Amsterdam Anton Pannekoek Inst Astron GRAPPA Amsterdam Netherlands;

Univ Adelaide Sch Phys Sci Adelaide SA Australia;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Savoie Mt Blanc Univ Grenoble Alpes Lab Annecy Phys Particules CNRS LAPP Annecy France;

North West Univ Ctr Space Res Potchefstroom South Africa;

Heidelberg Univ Landessternwarte Heidelberg Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Inst Fizyki Jadrowej PAN Krakow Poland|Heidelberg Univ Landessternwarte Heidelberg Germany;

Max Planck Inst Kernphys Heidelberg Germany;

Univ Tokyo Inst Adv Study UTIAS Kavli Inst Phys & Math Universe WPI Kashiwa Chiba Japan;

North West Univ Ctr Space Res Potchefstroom South Africa;

Max Planck Inst Kernphys Heidelberg Germany;

Polish Acad Sci Nicolaus Copernicus Astron Ctr Warsaw Poland;

Univ Paris Diderot PSL Res Univ Observ Paris LUTH CNRS Meudon France;

Friedrich Alexander Univ Erlangen Nurnberg Erlangen Ctr Astroparticle Phys Erlangen Germany;

Max Planck Inst Kernphys Heidelberg Germany;

North West Univ Ctr Space Res Potchefstroom South Africa;

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1. ULTRA-HIGH ENERGY COSMIC-RAY ACCELERATION IN THE JET OF CENTAURUS A [J] . Mitsuru Honda The Astrophysical journal . 2009,第2期

机译：CENTURUS A射流的超高能宇宙射线加速
2. The X-Ray Jet in Centaurus A: Clues to the Jet Structure and Particle Acceleration [J] . Jun Kataoka1, ?ukasz Stawarz23, Felix Aharonian2, The Astrophysical journal . 2008,第1期

机译：半人马座A中的X射线射流：射流结构和粒子加速的线索
3. THE X-RAY JET IN CENTAURUS A: CLUES TO THE JET STRUCTURE AND PARTICLE ACCELERATION [J] . Jun Kataoka, Lukasz Stawarz, Felix Aharonian, The Astrophysical journal . 2006,第1Pt1期

机译：人马座的X射线射流：射流结构和粒子加速的线索
4. Particle transport and stochastic acceleration in the giantlobes of Centaurus A [C] . Stephen OSullivan International Symposium on the Recent Progress of Ultra-high Energy Cosmic Ray Observation . 2011

机译：粒子传输和中心的颗粒式锥体A
5. Determining the Acceleration Mechanism and Magnetic Topological Structure of Coronal Jets: Evidence for Multiple Acceleration Mechanisms [D] . Farid, Samaiyah I. 2020

机译：确定冠状动脉的加速机制和磁性拓扑结构：多种加速机制的证据
6. The acceleration and collimation of jets. [O] . M C Begelman 1995

机译：喷嘴的加速和准直。
7. Resolving acceleration to very high energies along the jet of Centaurus A [O] . H. Abdalla, R. Adam, F. Aharonian, 2020

机译：解决沿着滨海射流的加速度到非常高的能量a

Resolving acceleration to very high energies along the jet of Centaurus A

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