High-Energy Emission from Pulsars and their Systems

The aim of the inaugural meeting of the Sant Cugat Forum on Astrophysics was to address, in a global context, the current understanding of and challenges in high-energy emissions from isolated and non-isolated neutron stars, and to confront the theoretical picture with observations of both the Fermi satellite and the currently operating ground-based Cherenkov telescopes. Participants have also discussed the prospects for possible observations with planned instruments across the multi-wavelength spectrum (e.g. SKA, LOFAR, E-VLT, IXO, CTA) and how they will impact our theoretical understanding of these systems.
In keeping with the goals of the Forum, this book not only represents the proceedings of the meeting, but also a reflection on the state-of-the-art in the topic.

• Cherenkov Telescopes
• Fermi Large Area Telescope
• Gamma y-ray Pulsars
• High-energy astrophysics
• Magnetars
• Neutron Stars
• Particle Astrophysics
• Pulsar Magnetospheres
• Pulsar Timing
• Pulsars
• Radio pulsars

• Inst. Ciències de l'Espai, CSIC Bellaterra, Bellaterra, Spain

  Diego F. Torres, Nanda Rea

Policies and ethics