Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2010-08-03
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
8 pages, 11 figures; invited talk at the conference "Steady Jets and Transient Jets, Characteristics and Relationship", held i
Scientific paper
Gamma-ray binaries are suitable sources to study high-energy processes in jets and outflows in general. In the last years, there has been a lot of activity in the field of gamma-ray binaries to identify the different factors that shape their non-thermal spectra, which ranges from radio to very high energies, as well as their lightcurves. In this work, I discuss the main aspects of the non-thermal emission in this class of objects, which presently includes high-mass microquasars, high-mass binaries hosting a non-accreting pulsar and, probably, massive star binaries; few potential candidates to be gamma-ray binaries are also presented. Finally, the importance of gamma-ray absorption is discussed, and the main physical ingredients, which are likely involved in the non-thermal radiation in gamma-ray binaries, are briefly considered.
No associations
LandOfFree
Spectral energy distribution of gamma-ray binaries: Sources and Processes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Spectral energy distribution of gamma-ray binaries: Sources and Processes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral energy distribution of gamma-ray binaries: Sources and Processes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-615068