Abstract
During my thesis, I studied three of the best microquasar candidates to emit at VHE: Cygnus X-1, Cygnus X-3 and V404 Cygni. For the first time, we firmly detected Cygnus X-1 in the HE regime owing to the analysis of the 7.5 years of pass 8 textitFermi data. This analysis allowed us to determine that HE gamma-ray emission only occurs during the HS and most likely associated to the relativistic jets. In turn, we found a hint of orbital modulation, which could constrain the gamma-ray emission site between \(10^{11}\)–\(10^{13}\) cm from the BH produced by anisotropic IC on the stellar photon field.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2018 Springer Nature Switzerland AG
About this chapter
Cite this chapter
Fernández Barral, A. (2018). Summary and Concluding Remarks. In: Extreme Particle Acceleration in Microquasar Jets and Pulsar Wind Nebulae with the MAGIC Telescopes. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-97538-2_11
Download citation
DOI: https://doi.org/10.1007/978-3-319-97538-2_11
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-319-97537-5
Online ISBN: 978-3-319-97538-2
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)