collaborators

6 papers

astro-ph.HE2025

The peculiar disk evolution of 4U 1630--472 observed by Insight-HXMT during the 2022 and 2023 outbursts

Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui +10

We study the spectral properties of the black hole X-ray transient binary 4U 1630--472 during the 2022 and 2023 outbursts with Insight-HXMT observations. We find that the outbursts…

astro-ph.HE2025

Insight-HXMT, NICER and NuSTAR views to the newly discovered black hole X-ray binary Swift J151857.0--572147

Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui +10

The systematic properties are largely unknown for the black hole X-ray binary Swift J151857.0--572147 newly discovered in the 2024 outburst. The nature of a black hole can be compl…

astro-ph.HE2025

NICER, NuSTAR and Insight-HXMT views to black hole X-ray binary SLX 1746--331

Jing-Qiang Peng, Shu Zhang, Qing-Cang Shui +13

We study the spectral and temporal properties of the black hole X-ray transient binary SLX 1746--331 during the 2023 outburst with NICER, NuSTAR, and Insight-HXMT observations. Thr…

astro-ph.HE2025

Insight-HXMT observations on thermonuclear X-ray bursts from 4U~1608--52 in 2022: the accretion rate dependent anisotropy of burst emission

Yu-Peng Chen, Shu Zhang, Long Ji +10

Thermonuclear X-ray bursts occur on the surface of an accreting neutron star (NS), and their characteristics and interplay with the surrounding circumstance could be a clue to unde…

astro-ph.HE2024

A Phase-resolved View of "Heartbeat"-like variability in IGR J17091-3624 During the 2022 Outburst

Qing-Cang Shui, Shu Zhang, Jing-Qiang Peng +9

IGR J17091-3624, in addition to GRS 1915+105, is the only black hole X-ray binary that displays ``heartbeat"-like variability characterized by structured flares with high amplitude…

astro-ph.HE2024

Phase-resolved Spectroscopy of Low-frequency Quasi-periodic Oscillations from the Newly Discovered Black Hole X-ray Binary Swift J1727.8-1613

Qing-Cang Shui, Shu Zhang, Jiang-Qiang Peng +14

Low-frequency quasi-periodic oscillations (LFQPOs) are commonly observed in X-ray light curves of black hole X-ray binaries (BHXRBs); however, their origin remains a topic of debat…