http://arxiv.org/abs/1803.03641
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.
T. Belloni
Tue, 13 Mar 2018
53/61
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)
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