INAF - Osservatorio Astronomico di Brera - Merate
(Image Credit: IPAC-Caltech)
Active galactic nuclei (AGN) are very bright regions at the center of some galaxies, powered by supermassive black holes. Some AGN produce narrow, fast jets of plasma that travel at nearly the speed of light — these are called relativistic jets. We study these jets to understand how they form, how they accelerate particles, and how they affect their surroundings. By looking at the light they emit — from radio waves to gamma rays — we explore the extreme physics happening near the black holes at the heart of active galaxies.
Relativistic MHD simulations
Magnetic turbulence & instabilities
Visualize jet structures
Radiation models
Polarization
Particle acceleration mechanisms
MAGIC, CTA, LST and ASTRI collaborations
Gamma ray detection and analysis
Multiwavelength campaigns
Dr. Gianluigi Bodo (INAF OA Torino)
Prof. Paolo Coppi (Yale University)
Dr. Agnese Costa (INAF OA Torino)
Dr. Giorgio Galanti (INAF-IASF)
Dr. Marco Landoni (INAF OA Brera)
Dr. Paola Rossi (INAF OA Torino)
Dr. Emanuele Sobacchi (GSSI)
Dr. Agnese Costa(Ph.D. Student, Insubria Univeristy)
Dr. Chiara Righi (PhD Student, Insubria University / Postdoctoral Researcher)
Dr. Giorgio Galanti (Postdoctoral Researcher)
Dr. Emanuele Sobacchi (Postdoctoral Researcher)