Accreting Millisecond X-Ray Pulsars
A. Patruno (Leiden/ASTRON), A. L. Watts (Univ. Amsterdam)

TL;DR
This review summarizes fifteen years of discoveries and observations of Accreting Millisecond X-Ray Pulsars, highlighting their significance in understanding extreme physics, plasma-magnetic interactions, and thermonuclear processes.
Contribution
It provides a comprehensive overview of observational and theoretical advances in AMXPs, emphasizing multi-wavelength data and insights into accretion, pulse formation, and burst phenomena.
Findings
Enhanced understanding of plasma-magnetic field interactions
Insights into thermonuclear burst oscillations
Refined models of accretion torque and pulse formation
Abstract
Accreting Millisecond X-Ray Pulsars (AMXPs) are astrophysical laboratories without parallel in the study of extreme physics. In this chapter we review the past fifteen years of discoveries in the field. We summarize the observations of the fifteen known AMXPs, with a particular emphasis on the multi-wavelength observations that have been carried out since the discovery of the first AMXP in 1998. We review accretion torque theory, the pulse formation process, and how AMXP observations have changed our view on the interaction of plasma and magnetic fields in strong gravity. We also explain how the AMXPs have deepened our understanding of the thermonuclear burst process, in particular the phenomenon of burst oscillations. We conclude with a discussion of the open problems that remain to be addressed in the future.
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