activity
20022024
most citedA Neutron Star-White Dwarf Binary Model for Repeating Fast Radio Burst 121102

78 citations · 561 across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2024

A New Model for the Extragalactic Radio Sky at Low Frequency Calibrated Using the LOFAR Two-metre Survey

Jinyang Lin, Zhenghao Zhu, Renyi Ma +2

Building the radio sky template are crucial for detecting the 21 cm emission line signal from the Epoch of Reionization (EoR), as well as for other cosmological research endeavors.…

astro-ph.HE2023★ 1 cited

The width-flux relation of the broad iron line during the state transition of the black hole X-ray binaries

Hang-Ying Shui, Fu-Guo Xie, Zhen Yan +1

The observation of varying broad iron lines during the state transition of the black hole X-ray binaries (BHXBs) have been accumulating.In this work, the relation between the norma…

astro-ph.HE2019★ 24 cited

A global solution to a slim accretion disk with radiation-driven outflows

Junjie Feng, Xinwu Cao, Wei-Min Gu +1

The thickness of a slim disk is determined by the balance between the radiation force and the vertical component of the gravity of the black hole (BH). It was found that vertical g…

astro-ph.HE2018★ 42 cited

Spectral Energy Distribution of the inner accretion flow around Sgr A* -- Clue for a weak outflow in the innermost region

Ren-Yi Ma, Shawn R. Roberts, Ya-Ping Li +1

Sgr A* represents a unique laboratory for the detailed study of accretion processes around a low-luminosity supermassive black hole (SMBH). Recent X-ray observations have allowed f…

astro-ph.GA2018★ 8 cited

XMM-Newton Survey of Local OVII Absorption Lines in the Spectra of Galactic X-ray Sources

Yang Luo, Taotao Fang, Renyi Ma

The detection of highly ionized metal absorption lines in the X-ray spectra of the Galactic X-ray binaries (XRBs) implies the distribution of hot gas along the sightline toward the…

astro-ph.HE2018★ 3 cited

The Profiles of Fe Kα Line From the Inhomogeneous Accretion Flow

Xiao-Di Yu, Ren-Yi Ma, Ya-Ping Li +2

The clumpy disc, or inhomogeneous accretion flow, has been proposed to explain the properties of accreting black hole systems. However, the observational evidences remain to be exp…