Plasma Science Hub

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14

AG2024 Splinter Meeting: The Physics behind the Multimessenger Emissions of Active Galactic Nuclei

Together with our colleagues of  FOR5195 - Relativistic Jets in Active Galaxies we are organizing a splinter meeting at the Annual Meeting of the German Astronomical Society.

This year, the annual meeting will be hosted at the University of Cologne from September 09-13, 2024.

Our joint splinter meeting comprises all aspects of multi-messenger AGN research to understand the processes which produce electromagnetic radiation, neutrinos and cosmic rays. With this approach, we will foster discussions on the physical properties, interaction mechanisms and evolution of AGN as well as how AGN influence and shape their environment.

For more information, please have a look at our meeting's page!