Particle acceleration and magnetic field amplification in hotspots of FR II galaxies: The case study 4C74.26
It has been suggested that relativistic shocks in extragalactic sources may accelerate the most energetic cosmic rays. However, recent theoretical advances indicating that relativistic shocks are probably unable to accelerate particles to energies much larger than a PeV cast doubt on this. In the pr...
المؤلفون الرئيسيون: | Araudo, A, Bell, A, Blundell, K |
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التنسيق: | Journal article |
منشور في: |
Argentinian Astronomical Society
2016
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مواد مشابهة
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Particle acceleration and magnetic field amplification in the jets of 4C74.26
حسب: Araudo, A, وآخرون
منشور في: (2015) -
The luminous X-ray hotspot in 4C 74.26: synchrotron or inverse-Compton
emission?
حسب: Erlund, M, وآخرون
منشور في: (2007) -
A JET IN THE NUCLEUS OF THE GIANT QUASAR 4C-74.26
حسب: Pearson, T, وآخرون
منشور في: (1992) -
Evidence that the maximum electron energy in hotspots of FR II galaxies is not determined by synchrotron cooling
حسب: Araudo, A, وآخرون
منشور في: (2016) -
Evidence that the maximum electron energy in hotspots of FR II galaxies is not determined by synchrotron cooling
حسب: Araudo, A, وآخرون
منشور في: (2016)