Our Research

Pulsar Wind Nebulae (PWNe) are bubbles of relativistic plasma arising from the confinement of a pulsar's wind ... [more]

Bow shock Pulsar Wind Nebulae (BSPWNe) form when a fast moving pulsar interact with the ambient medium, after having leaved ... [more]

After the explosion of a star, the evolution of the stellar debris and its interaction with the surroundings gives rise to a number of fascinating phenomena... [more]

Cosmic rays are energetic charged particles that reach us from the Cosmos, carrying information on the most energetic sources ...[more]

Gamma-Ray Bursts (GRBs) are flashes of gamma rays related to extremely energetic explosions taking place in distant galaxies... [more]

Neutron Stars (NSs) are the most compact objects in the universe endowed with an internal structure... [more]

Accurate and robust Riemann solvers for SRMHD requiring fewer eigen-modes have been also recently developed... [more]

Lorem Ipsum [more]