15–19 Aug 2022
Niels Bohr Institute
Europe/Copenhagen timezone

Interaction between a central radio galaxy and the ICM

17 Aug 2022, 13:45
25m

Speaker

Paul Nulsen (Harvard-Smithsonian Center for Astrophysics)

Description

Chandra observations of radio galaxies hosted by the central galaxy of a group or cluster continue to provide insights into the makeup of jets and lobes and their interactions with the environment. My main focus will be implications of the rich X-ray and radio structure observed in Cygnus A. Among other things, I will argue that the feature known as the X-ray jet in Cygnus A is formed by encounters between gas clouds and the jet, which leave trails of remnant plasma scattered along the path of the jet. I will also discuss early results of numerical simulations for the formation of the hole found in the X-ray emission around the primary hotspot in the eastern lobe of Cygnus A.

Primary authors

John ZuHone (Center for Astrophysics | Harvard & Smithsonian) Paul Nulsen (Harvard-Smithsonian Center for Astrophysics)

Presentation materials