papers

Publications (41)

astro-ph.HE2021

Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070

Bei You, Yuoli Tuo, Chengzhe Li +123

A black hole X-ray binary produces hard X-ray radiation from its corona and disk when the accreting matter heats up. During an outburst, the disk and corona co-evolves with each ot…

cond-mat.str-el2025

Abnormal planar Hall effect and disentanglement of incoherent and coherent transport in a Kondo lattice

Shuo Zou, Hai Zeng, Zhuo Wang +7

The nature of localized-itinerant transition in Kondo lattice systems remains a mystery despite intensive investigations in past decades. While it is often identified from the cohe…

cond-mat.str-el2024

Al NMR study of the magnetic Weyl semimetal CeAlGe

Zhuo Wang, Xiaobo He, Fangjun Lu +4

Motivated by the recent observations of electronic correlation effect [M. Corasaniti \textit{et al}., Phys. Rev. B \textbf{104}, L121112 (2021)] and topology-stabilized magnetic fl…

astro-ph.HE2024

Evidence for a nearly orthogonal rotator in GX 301--2 with phase-resolved cyclotron resonant scattering features

Xiao Chen, Yuanze Ding, Wei Wang +8

Cyclotron resonant scattering features (CRSFs) are the absorption features in the X-ray spectra of strongly magnetized accretion neutron stars (NSs), which are probably the most re…

astro-ph.HE2026

X-rays breaking out of pre-explosion ejecta mark a supernova's first light

Weimin Yuan, Qiu-Ju Huang, Jin-Ping Zhu +130

Massive stars die as core-collapse supernovae, whose optical light emerges days after the implosion. Theory predicts that the initial collapse-driven shock, upon breaking through t…

astro-ph2008

Progress on multi-waveband observations of supernova remnants

Xuejuan Yang, Fangjun Lu, Wenwu Tian

The development of observational techniques has inriched our knowledge of supernova remnants. In this paper, we review the main progresses in the last decade, including new discove…