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Updated: Jul 23, 2026

Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation
Published on: October 30, 2012
Particle accelerators in the hot spots of radio galaxy 3C 445, imaged with the VLT
M Almudena Prieto1, Gianfranco Brunetti, Karl-Heinz Mack
1European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany. aprieto@eso.org
Abstract:
Hot spots (HSs) are regions of enhanced radio emission produced by supersonic jets at the tip of the radio lobes of powerful radio sources. Obtained with the Very Large Telescope (VLT), images of the HSs in the radio galaxy 3C 445 show bright knots embedded in diffuse optical emission distributed along the post-shock region created by the impact of the jet into the intergalactic medium. The observations reported here confirm that relativistic electrons are accelerated by Fermi-I acceleration processes in HSs. Furthermore, both the diffuse emission tracing the rims of the front shock and the multiple knots demonstrate the presence of additional continuous re-acceleration processes of electrons (Fermi-II).
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