| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8133088 | Astroparticle Physics | 2013 | 16 Pages |
Abstract
⺠CTA will provide the best sensitivity to study variable, compact VHE sources. ⺠CTA will provide a ten-fold increase in the number of known gamma-ray binaries. ⺠Broad dynamical range is essential to probe non-thermal physics. ⺠Good angular resolution is required to resolve large scale outflow interactions. ⺠Subarray observations are crucial for long-term monitoring of known systems.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
J.M. Paredes, W. Bednarek, P. Bordas, V. Bosch-Ramon, E. De Cea del Pozo, G. Dubus, S. Funk, D. Hadasch, D. Khangulyan, S. Markoff, J. Moldón, P. Munar-Adrover, S. Nagataki, T. Naito, M. de Naurois, G. Pedaletti, O. Reimer, M. Ribó, A.A. Zdziarski,