X-ray emission from black-hole and neutron-star binaries
High Energy Astrophysical Phenomena
2018-03-13 v1
Abstract
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.
Keywords
Cite
@article{arxiv.1803.03641,
title = {X-ray emission from black-hole and neutron-star binaries},
author = {Tomaso M. Belloni},
journal= {arXiv preprint arXiv:1803.03641},
year = {2018}
}
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)