A magnetar is a type of neutron star with an extremely powerful magnetic field. The magnetic field decay powers the emission of high-energy electromagnetic radiation, particularly X-rays and gamma rays. The magnetar hypothesis has become widely accepted as a likely explanation for soft gamma repeaters(SGRs) and anomalous X-ray pulsars (AXPs).
Lectures will be given by:
- R. Turolla (Padova University & INFN)
- A. Bonanno (INAF & INFN)
You can register for the lectures by using the registration form on your left. Registration deadline is September 14, 2015.
