Abstract
We apply to LS 5039 a new model where the microquasar jet is dynamically dominated by cold protons and radiatively dominated by relativistic leptons. Recent observational results on this microquasar, altogether with previous observational findings, are interpreted in the context of this model. We compute the spectral energy distribution of radiation, making some predictions about the amount of emission produced at the highest energies, where no observational data is available yet.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
