Accès ouvert
2026
article
OpenAlex
W Li, Shiyu Zhang, Qing-Cang Shui, Yupeng Chen et autres
Abstract We analyze 10 XMM-Newton observations of the narrowline Seyfert 1 galaxy RE J1034+396 to investigate the origin of its quasiperiodic oscillation (QPO). Using the Hilbert–Huang Transform, we perform the first systematic phase-resolved X-ray spectral analysis of this source. We report that …
cn, ru, au
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Accès ouvert
2026
dataset
OpenAlex
M. Y. Ge, Liu C.Z, Shuang‐Nan Zhang, F. J. Lu et autres
cn
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Accès ouvert
2026
article
OpenAlex
Sheng-Lun Xie, Aming Chen, Yun-Wei Yu, S. L. Xiong et autres
Abstract In theory, burst activity of the magnetar can lead to the formation of fireballs trapped by the magnetic field and corotating with the star. However, smoking-gun observational evidence of the fireball is elusive. We envisage that the fireball emission should occasionally …
cn, rs
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Accès ouvert
2026
article
OpenAlex
Hongling Peng, Shanshan Weng, M. Y. Ge, Shiqi Zhou et autres
Abstract Anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) are believed to be manifestations of magnetars. Typically, AXPs exhibit higher X-ray luminosities, whereas SGRs are generally fainter and display significantly high signal-to-noise ratios only during their outburst phases. In this work, …
cn, de
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Accès ouvert
2026
article
OpenAlex
Wen-Zhong Li, Shu Zhang, Qing-Cang Shui, Yupeng Chen et autres
Abstract 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 during 2020–2021. Our analysis reveals that the QPO in the source exhibits two mutually convertible lag-energy modes: …
Accès ouvert
2026
article
OpenAlex
Yu-Feng Luo, Shanshan Weng, Qing-Zhong Liu, M. Y. Ge et autres
Abstract PSR J2032+4127 is the only gamma-ray binary that exhibits pulsations in gamma rays. Previous research has indicated that the pulsar and the Be star MT91 213 orbit each other in a highly eccentric orbit with an extremely long period, with the …
Accès ouvert
2025
article
OpenAlex
Yupeng Chen, Long Ji, Shu Zhang, Shuang‐Nan Zhang et autres
Abstract The thermonuclear X-ray burster, 4U 0614+09, which is located at a distance of ∼3 kpc, serves as a valuable laboratory for studying the interaction between thermonuclear X-ray bursts and the surrounding accretion environment. By analyzing the archived data from NICER and …
Accès ouvert
2025
article
OpenAlex
Wai Ling Wu, Fei Xie, Long Ji, M. Y. Ge et autres
Abstract Vela X-1 is one of the most archetypal wind-fed X-ray pulsars (XRPs), and the emergence of its orthogonal polarization states reveals distinctive polarimetric properties. Using data from Imaging X-ray Polarimetry Explorer observations of Vela X-1, we perform a polarization analysis of …
Accès ouvert
2025
preprint
OpenAlex
Wai Ling Wu, Fei Xie, Long Ji, M. Y. Ge et autres
Vela X-1 is one of the most archetypal wind-fed X-ray pulsars (XRPs), and the emergence of its orthogonal polarization states reveals distinctive polarimetric properties. Using data from Imaging X-ray Polarimetry Explorer (IXPE) observations of Vela X-1, we perform a polarization analysis of …
Accès ouvert
2025
article
OpenAlex
Min Wei, Xiang Ma, Liang Zhang, X. H. Li et autres
Abstract We present a detailed analysis of the evolution of type-C quasiperiodic oscillations (QPOs) observed during the flaring state of the recently discovered black hole X-ray binary Swift J1727.8–1613, utilizing data from the Insight Hard X-ray Modulation Telescope. By examining the relation …
cn
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Accès ouvert
2025
article
OpenAlex
W. T. Ye, Peng Zhang, M. Y. Ge, Liqiang Qi et autres
Abstract Soft γ -ray pulsars featuring broad single peaks exhibit different observational properties compared to ordinary double-peaked high-energy pulsars. These two types of pulsars are considered to be the result of different viewing angles. Therefore, the radiation characteristics of soft γ -ray …
Accès ouvert
2025
article
OpenAlex
Lei Zhang, Li Chen, Yuanyue Pan, Wenhui Yu et autres
We present a detailed analysis of seven thermonuclear X-ray bursts from Terzan 5 X–3/Swift J174805.3–244637 detected by NICER during the source’s 2023 outburst. Our analysis reveals a clear evolution of burst properties, identifying four non-photospheric radius expansion (non-PRE) bursts, one PRE candidate …
cn
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