collaborators

13 papers

astro-ph.HE2026

Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262

Lingda Kong, Xiaohang Dai, Andrea Santangelo +12

Accretion onto strongly magnetized neutron stars is commonly interpreted using quasi-steady models, in which the accretion-column structure adjusts smoothly to the mass inflow rate…

astro-ph.HE2026

First detection of X-ray polarization from the long-period X-ray pulsar 4U 1954+319

Alexander Salganik, Lingda Kong, Sofia V. Forsblom +6

We report the first detection of X-ray polarization with the Imaging X-ray Polarimetry Explorer from the X-ray pulsar (XRP) 4U 1954319. The source belongs to an extremely rare c…

astro-ph.HE2026

A clean broad iron line in GS 1354--64 as seen by XRISM

Honghui Liu, Lingda Kong, Oluwashina K. Adegoke +13

We present a spectroscopic analysis of XRISM and NuSTAR observations of the black hole X-ray binary GS~1354--64 during its 2026 outburst. A total number of 3.5 million photons are…

astro-ph.HE2026

Discovery of a New Spectral Transition in Swift J0243.6+6124 in the Sub-Eddington Regime

Bo-Yan Chen, Shu Zhang, Qing-Cang Shui +9

We conduct a detailed spectral analysis of the Galactic ultraluminous X-ray pulsar Swift J0243.6+6124 in its sub-Eddington regime, using Insight-HXMT and NICER observations during…

astro-ph.HE2026

Investigation on Quasi-periodic Oscillation Phase Lag of RE J1034+396

Wen-Zhong Li, Shu Zhang, Qing-Cang Shui +9

We conduct an in-depth study of the quasi-periodic oscillation (QPO) properties of RE J1034+396, by constructing QPO phase-folded light curves from 10 XMM-Newton observations durin…

astro-ph.HE2026

Long-term evolution of cyclotron resonant scattering features in the accreting pulsar Vela X-1: A pulse-to-pulse approach

Yu-Jia Du, Peng-Ju Wang, Lorenzo Ducci +5

We investigated the long-term evolution of the cyclotron line energy, as well as the relationship between cyclotron line energy and luminosity in the high-mass X-ray binary Vela X-…