Magic Constraints on γ-ray Emission from Cygnus X-3
Cygnus X-3 is a microquasar consisting of an accreting compact object orbiting around a Wolf-Rayet star. It has been detected at radio frequencies and up to high-energy γ rays (above 100 MeV). However, many models also predict a very high energy (VHE) emission (above hundreds of GeV) when the source displays relativistic persistent jets or
Aleksić, J. et al.
Fecha de publicación:
9
2010