activity
19992023
most citedMagnetic field reversal in the turbulent environment around a repeating fast radio burst

121 citations · 979 across the 47 of their papers we have counts for

collaborators

47 papers

astro-ph.HE2023★ 70 cited

A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism

Weiwei Zhu, Heng Xu, Dejiang Zhou +34

The megajansky radio burst, FRB 20200428, and other bright radio bursts detected from the Galactic source SGR J1935+2154 suggest that magnetars can make fast radio bursts (FRBs), b…

astro-ph.HE2023★ 1 cited

An apparent positive relation between spin and orbital angular momentum in X-ray binaries

Zhen Yan, Wenda Zhang, Wenfei Yu

The origin of current angular momentum (AM) of the black hole (BH) in X-ray binary (XRB) is still unclear, which is related with the birth and/or the growth of the BH. Here we coll…

astro-ph.HE2023

Temporal and Spectral Properties of the Persistent Radio Source Associated with FRB 20190520B with the VLA

Xian Zhang, Wenfei Yu, Casey Law +12

Among more than 800 known fast radio bursts (FRBs), only two, namely FRB 20121102A and FRB 20190520B, are confirmed to be associated with a persistent radio sources (PRS). Here we…

astro-ph.HE2023★ 14 cited

Low Frequency Quasi-periodic Oscillation in MAXI J1820+070: Revealing distinct Compton and Reflection Contributions

Chenxu Gao, Zhen Yan, Wenfei Yu

X-ray low frequency quasi-periodic oscillations (LFQPOs) of black hole X-ray binaries, especially those type-C LFQPOs, are representative timing signals of black hole low/hard stat…

astro-ph.HE2022★ 121 cited

Magnetic field reversal in the turbulent environment around a repeating fast radio burst

Reshma Anna-Thomas, Liam Connor, Shi Dai +27

Fast radio bursts (FRBs) are brief, intense flashes of radio waves from unidentified extragalactic sources. Polarized FRBs originate in highly magnetized environments. We report ob…

astro-ph.HE2021

Power spectral properties of the soft spectral states in four black hole transients

Dongming Mao, Wenfei Yu

The X-ray variability in the soft X-ray spectral state of black hole binaries is primarily characterized by a power-law noise (PLN), which is thought to originate from the propagat…