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X-ray emission from black-hole and neutron-star binaries

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arxiv 1803.03641 v1 pith:P6GWT3OB submitted 2018-03-09 astro-ph.HE

X-ray emission from black-hole and neutron-star binaries

Tomaso M. Belloni (INAF - Osservatorio Astronomico di Brera) This is my paper
classification astro-ph.HE
keywords binariesblack-holeneutron-starx-raybehaviourchaptercharacteristicsconcentrating
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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.

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  1. Search for the Highest-energy Quasiperiodic Oscillation in the Black Hole X-Ray Binary Candidate Swift J1727.8-1613

    astro-ph.HE 2026-05 unverdicted novelty 7.0

    First detection of QPOs above 250 keV in Swift J1727.8-1613 with up to 8.9 sigma significance, showing decreasing rms and increasing soft lags that suggest a geometric origin from small-scale jet precession.