The TeV-emitting radio galaxy 3C 264. VLBI kinematics and SED modeling

@inproceedings{Boccardi2019TheTR,
  title={The TeV-emitting radio galaxy 3C 264. VLBI kinematics and SED modeling},
  author={Biagina Boccardi and Giulia Migliori and Paola Grandi and Eleonora Torresi and Florent Mertens and Vassilis Karamanavis and Roberto Angioni and Cristian Vignali},
  year={2019}
}
  • Biagina Boccardi, Giulia Migliori, +5 authors Cristian Vignali
  • Published 2019
  • Physics
  • In March 2018, Mukherjee (2018) reported the detection by VERITAS of very-high-energy emission (VHE; > 100 GeV) from 3C 264. This is the sixth, and second most distant, radio galaxy ever detected in the TeV regime. In this article we present a radio and X-ray analysis of the jet in 3C 264. We determine the main physical parameters of the parsec-scale flow and explore the implications of the inferred kinematic structure for radiative models of this gamma-ray emitting jet. The radio data set is… CONTINUE READING

    Create an AI-powered research feed to stay up to date with new papers like this posted to ArXiv