activity
20192026
most citedA dynamically discovered and characterized non-accreting neutron star -- M dwarf binary candidate

31 citations · 44 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2026

Photoionization of the Composite Nebula Surrounding NGC 5408 X-1: Implications for Beamed Emission

Jing Guo, Hua Feng, Roberto Soria +4

NGC 5408 X-1 is one of the best studied ultraluminous X-ray sources (ULXs) and is surrounded by a photoionized nebula. Previous optical spectroscopy established the presence of str…

astro-ph.HE2022★ 4 cited

Bubble in the Whale: Identifying the Optical Counterparts and Extended Nebula for the Ultraluminous X-ray Sources in NGC 4631

Jing Guo, Jianfeng Wu, Hua Feng +9

We present a deep optical imaging campaign on the starburst galaxy NGC 4631 with CFHT/MegaCam. By supplementing the HST/ACS and Chandra/ACIS archival data, we search for the optica…

astro-ph.SR2022★ 31 cited

A dynamically discovered and characterized non-accreting neutron star -- M dwarf binary candidate

Tuan Yi, Wei-Min Gu, Zhi-Xiang Zhang +26

Optical time-domain surveys can unveil and characterize exciting but less-explored non-accreting and/or non-beaming neutron stars (NS) in binaries. Here we report the discovery of…

astro-ph.HE2021★ 3 cited

The Disk Veiling Effect of the Black Hole Low-Mass X-ray Binary A0620-00

Wan-Min Zheng, Qiaoya Wu, Jianfeng Wu +15

The optical light curves of quiescent black hole low-mass X-ray binaries often exhibit significant non-ellipsoidal variabilities, showing the photospheric radiation of the companio…

astro-ph.HE2019★ 6 cited

Thick-disc model to explain the spectral state transition in NGC 247

Jing Guo, Mouyuan Sun, Wei-Min Gu +1

We propose the thick-disc model of Gu et al. 2016 to interpret the transition between soft ultraluminous state (SUL) and supersoft ultraluminous (SSUL) state in NGC 247. As accreti…