activity
20152026
most citedThe Biases of Optical Line-Ratio Selection for Active Galactic Nuclei, and the Intrinsic Relationship between Black Hole Accretion and Galaxy Star Formation

149 citations · 1.4k across the 73 of their papers we have counts for

collaborators
Showing 2022Show all

9 papers · 1 filter

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.HE2022★ 15 cited

One-off and Repeating Fast Radio Bursts: A Statistical Analysis

Hao-Yan Chen, Wei-Min Gu, Mouyuan Sun +1

According to the number of detected bursts, fast radio bursts (FRBs) can be classified into two categories, i.e., one-off FRBs and repeating ones. We make a statistical comparison…

astro-ph.SR2022★ 12 cited

A White Dwarf-Main Sequence Binary Unveiled by Time-Domain Observations from LAMOST and TESS

Ling-Lin Zheng, Wei-Min Gu, Mouyuan Sun +16

We report a single-lined white dwarf-main sequence binary system, LAMOST J172900.17+652952.8, which is discovered by LAMOST's medium resolution time-domain surveys. The radial velo…

astro-ph.SR2022★ 13 cited

A long-period pre-ELM system discovered from LAMOST medium-resolution survey

Zhi-Xiang Zhang, Ling-Lin Zheng, Wei-Min Gu +16

We present LAMOST~J041920.07+072545.4 (hereafter J0419), a close binary consisting of a bloated extremely low mass pre-white dwarf (pre-ELM WD) and a compact object with an orbital…

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.HE2022★ 8 cited

Repeating Ultraluminous X-ray Bursts and Repeating Fast Radio Bursts: A Possible Association?

Hao-Yan Chen, Wei-Min Gu, Jin-Bo Fu +3

Ultraluminous X-ray bursts (hereafter ULXBs) are ultraluminous X-ray flares with a fast rise ( one minute) and a slow decay ( an hour), which are commonly observed in e…

astro-ph.HE2022★ 7 cited

Nucleosynthesis Contribution of Neutrino-dominated Accretion Flows to the Chemical Evolution of Active Galactic Nuclei

Yan-Qing Qi, Tong Liu, Zhen-Yi Cai +1

Recent observations of quasars show high line-flux ratios in their broad emission lines and the ratios appear to be independent of redshift up to , which indicate that…

astro-ph.HE2022★ 10 cited

Thermal Equilibrium Solutions of Black Hole Accretion Flows: Outflows VS Advection

Wen-Biao Wu, Wei-Min Gu, Mouyuan Sun

Observations and numerical simulations have shown that outflows generally exist in the accretion process. We revisit the thermal equilibrium solutions of black hole accretion flows…

astro-ph.GA2022★ 34 cited

Evidence for quasar fast outflows being accelerated at the scale of tens of parsecs

Zhicheng He, Guilin Liu, Tinggui Wang +14

Quasar outflows may play a crucial role in regulating the host galaxy, although the spatial scale of quasar outflows remain a major enigma, with their acceleration mechanism poorly…