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Agenda

Lectures on Magnetar

Sept 15-16, 2015

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).

 

Contatti

"La Società della Conoscenza in Abruzzo"

Laboratori Nazionali del Gran Sasso 

Servizio Alta Formazione

Via G. Acitelli, 22
67100 Assergi L’Aquila
tel. +39 0862 4371