Tomaso M. Belloni
Published 2018-03-09Version 1
In this chapter, I present the main X-ray observational characteristics of black-hole binaries and low magnetic field neutron-star binaries, concentrating on what can be considered similarities or differences, with particular emphasis on their fast-timing behaviour.
Comments: To appear in HIGH TIME RESOLUTION ASTROPHYSICS - XXVII Canary Islands Winter School of Astrophysics (ed. Tariq Shahbaz. Jorge Casares Vel\'azquez, Teodoro Mu\~noz Darias)
X-ray emission from black-hole binaries
Modulation Mechanism of TeV, GeV, and X-ray Emission in LS5039
States and transitions in black-hole binaries
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