Millihertz quasi-periodic oscillations in accreting X-ray pulsars

TL;DR

This review summarizes observational features and theoretical interpretations of millihertz quasi-periodic oscillations in accreting X-ray pulsars, highlighting recent findings and future research directions.

Contribution

It provides a comprehensive overview of mHz QPOs in X-ray pulsars, combining recent observational data with current theories and identifying challenges for future studies.

Findings

Identification of mHz QPOs in both low-mass and high-mass X-ray binaries

Summary of observational features from recent X-ray missions

Discussion of theoretical models and remaining challenges

Abstract

Accreting neutron stars exhibit pulsed X-rays and complex temporal variability across multi-wavelengths and different timescales. This variability could be driven by various physical processes including instability or inhomogeneous motions within the accretion flow, thermonuclear bursts on the neutron star surface. In this review, we present a concise overview of the observational features for millihertz (mHz) quasi-periodic oscillations (QPOs) at a frequency range of $\sim 1- 1000$ mHz observed in light curves of X-ray pulsars for both low-mass X-ray binaries and high-mass X-ray binaries, based on recent X-ray missions, e.g., NICER, Insight-HXMT and NuSTAR. We further summarize current theoretical interpretations, discuss remaining challenges and propose potential directions for future studies to advance the understanding of the nature and physical origin of these QPOs.