Exploring physics of rotation powered pulsars with sub-10 GeV imaging atmospheric Cherenkov telescopes
Preprint
- 1 August 2002
Abstract
We discuss the potential of future sub-10 GeV threshold imaging atmospheric Cherenkov telescope arrays for exploring the physics of rotation powered pulsars and their interactions with the ambient medium through relativistic winds and termination shocks.Keywords
All Related Versions
- Version 1, 2002-08-01, ArXiv
- Published version: New Astronomy, 8 (2), 85.
This publication has 0 references indexed in Scilit: