Speaker
Ana Laura Müller
(Astronomical Institute of the Czech Academy of Sciences)
Description
The collision of stellar winds with astrophysical plasmas could lead to the formation of strong shocks where particles could be accelerated. In this work, we study the interaction between the wind of a young stellar cluster and the jet of an active galactic nucleus. We present our results for the maximum energies that particles could achieve in this scenario, and discuss the production of non-thermal signatures and the possibility of detecting them with current and future instruments.
Primary author
Ana Laura Müller
(Astronomical Institute of the Czech Academy of Sciences)