Evidence that particle acceleration in hotspots of FR II galaxies is not constrained by synchrotron cooling
Nuclear and Particle Physics Proceedings 297-299 (2018) 242-248
Abstract:
© 2018 We study the hotspots of powerful radiogalaxies, where electrons accelerated at the jet termination shock emit synchrotron radiation. The turnover of the synchrotron spectrum is typically observed between infrared and optical frequencies, indicating that the maximum energy of non-thermal electrons accelerated at the shock is ≲ TeV for a canonical magnetic field of ∼100 μG. We show that this maximum energy cannot be constrained by synchrotron losses as usually assumed, unless the jet density is unreasonably large and most of the jet upstream energy goes to non-thermal particles. We test this result by considering a sample of hotspots observed at radio, infrared and optical wavelengths.Revival of the Magnetar PSR J1622-4950: Observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR
ASTROPHYSICAL JOURNAL 856:2 (2018) ARTN 180
SNe 2013K and 2013am: observed and physical properties of two slow, normal Type IIP events
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 475:2 (2018) 1937-1959
LOFAR 150-MHz observations of SS 433 and W 50
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 475:4 (2018) 5360-5377
RFI flagging implications for short-duration transients
Astronomy and Computing Elsevier 23 (2018) 103-114