Speaker
Rubén López Coto
(IAA - CSIC)
Description
The Crab Pulsar is one of the few pulsars detected from GeV up to TeV energies. This talk will review recent gamma-ray observations of the pulsar performed with Imaging Atmospheric Cherenkov Telescopes (IACTs) and analyze their implications for current theoretical models that aim to explain the Very High Energy (VHE) emission from this source.
Primary author
Rubén López Coto
(IAA - CSIC)
