Pulsars at the Highest Energies: Questions for AGILE, Fermi (GLAST) and Atmospheric Cherenkov Telescopes | Zendy

D. J. Thompson | Zendy; F. Aharonian | Zendy; Werner Hofmann | Zendy; Frank Rieger | Zendy

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Pulsars at the Highest Energies: Questions for AGILE, Fermi (GLAST) and Atmospheric Cherenkov Telescopes

Author(s) -

D. J. Thompson,

F. Aharonian,

Werner Hofmann,

Frank Rieger

Publication year - 2008

Publication title -

aip conference proceedings

Language(s) - English

Resource type - Conference proceedings

SCImago Journal Rank - 0.177

H-Index - 75

eISSN - 1551-7616

pISSN - 0094-243X

DOI - 10.1063/1.3076626

Subject(s) - cherenkov radiation , fermi gamma ray space telescope , physics , pulsar , agile software development , astronomy , astrophysics , optics , computer science , detector , software engineering

Observational studies of gamma‐ray pulsars have languished in recent years, while theoretical studies have made significant strides. Now, with new and improved gamma‐ray telescopes coming online, opportunities present themselves for dramatic improvements in our understanding of these objects. The new facilities and better modeling of processes at work in high‐energy pulsars will address a number of important open questions.

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