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 2024Show all

17 papers · 1 filter

astro-ph.GA2024

Reverberation Mapping of Two Variable Active Galactic Nuclei: Probing the Distinct Characteristics of the Inner and Outer Broad-line Regions

Hai-Cheng Feng, Sha-Sha Li, J. M. Bai +8

Current reverberation mapping (RM) studies primarily focus on single emission lines, particularly the \hb\ line, which may not fully reveal the geometry and kinematic properties of…

astro-ph.GA2024

A Short-lived Rejuvenation during the Decades-long Changing-look Transition in the Nucleus of Mrk 1018

Kai-Xing Lu, Yan-Rong Li, Qingwen Wu +13

Changing-look active galactic nuclei (CL-AGNs), characterized by emerging or disappearing of broad lines accompanied with extreme continuum flux variability, have drawn much attent…

astro-ph.HE2024

The disk reverberation mapping of the lensed quasar Q0957+561

Marcin Marculewicz, Mouyuan Sun, Zhixiang Zhang +1

The measurement of continuum time lags in lensed quasars can effectively probe the accretion physics of quasars. This is because microlensing observations of lensed quasars can pro…

astro-ph.GA2024

Could the inter-band lag of active galactic nucleus vary randomly?

Zhen-Bo Su, Zhen-Yi Cai, Jun-Xian Wang +18

The inter-band lags among the optical broad-band continua of active galactic nuclei (AGNs) have been intensively explored over the past decade. However, the nature of the lags rema…

astro-ph.GA2024

Rare Occasions: Tidal Disruption Events Rarely Power the AGNs Observed in Dwarf Galaxies

Joanne Tan, Guang Yang, Jonelle L. Walsh +6

Tidal disruption events (TDEs) could be an important growth channel for massive black holes in dwarf galaxies. Theoretical work suggests that the observed active galactic nuclei (A…

astro-ph.GA2024

How Long Will the Quasar UV/Optical Flickering Be Damped? II. the Observational Test

Guowei Ren, Shuying Zhou, Mouyuan Sun +1

The characteristic timescale at which the variability of active galactic nuclei (AGNs) turns from red noise to white noise can probe the accretion physics around supermassive black…

astro-ph.HE2024

Nucleosynthesis contribution of neutrino-dominated accretion flows to the solar neighborhood

Yan-Qing Qi, Tong Liu, Mouyuan Sun +1

The elemental abundances of stars reflect the complex enrichment history of the galaxy. To explore and explain the metal enrichment history of the cosmic environment near our solar…

astro-ph.GA2024★ 18 cited

Velocity-resolved Reverberation Mapping of Changing-look Active Galactic Nucleus NGC 4151 during Outburst Stage. II. Four Season Observation Results

Hai-Cheng Feng, Sha-Sha Li, J. M. Bai +7

We present the results of a four-year velocity-resolved reverberation mapping (RM) campaign of the changing-look active galactic nucleus (CL-AGN) NGC 4151 during its outburst phase…

astro-ph.HE2024★ 1 cited

Unprecedented Continuum Time Delay Variation Phenomenon in an Active Supermassive Black Hole

Shuying Zhou, Mouyuan Sun, Hai-Cheng Feng +12

Resolving the accretion disks and broad line regions (BLRs) of active galactic nuclei (AGNs) can probe the physics behind supermassive black holes (SMBHs) fueling and weigh SMBHs.…

astro-ph.GA2024★ 3 cited

Newly Discovered Changing-look Active Galactic Nuclei from SDSS and LAMOST Surveys

Qian Dong, Zhi-Xiang Zhang, Wei-Min Gu +2

Changing-look Active Galactic Nuclei (CL AGNs) exhibit drastic variations in broad emission lines (BELs), the mechanism of which remains unclear. Expanding the sample of CL AGNs is…

astro-ph.SR2024★ 1 cited

A Sample of Compact Object Candidates in Single-lined Spectroscopic Binaries from LAMOST Medium Resolution Survey

Hao-Bin Liu, Wei-Min Gu, Zhi-Xiang Zhang +3

The stellar spectra from LAMOST Medium Resolution Survey can be used to search for compact objects in binaries. The LAMOST DR10 catalog includes > 980, 000 targets with multiple me…

astro-ph.GA2024★ 13 cited

A new timescale-mass scaling for the optical variation of active galactic nuclei across the intermediate-mass to supermassive scales

Zhen-Bo Su, Zhen-Yi Cai, Mouyuan Sun +3

Variability of active galactic nuclei (AGNs) has long been servicing as an essential avenue of exploring the accretion physics of black hole (BH). There are two commonly used metho…

astro-ph.GA2024★ 7 cited

Optical Continuum Reverberation Mapping of a Candidate IMBH in a Nearby Seyfert 1 Galaxy

Wenwen Zuo, Hengxiao Guo, Jingbo Sun +25

To investigate the short-term variability and determine the size of the optical continuum emitting region of intermediate-mass black holes (IMBHs), we carried out high-cadence, mul…

astro-ph.HE2024

Sizes of active galactic nuclei inhomogeneous disks -- large in microlensing, small in reverberation mapping

Guowei Ren, Mouyuan Sun, Jun-Xian Wang +1

Magnetohydrodynamics (MHD) turbulence can drive significant temperature fluctuations in the accretion disk of an active galactic nucleus (AGN). As a result, the disk can be highly…

astro-ph.HE2024

Stellar black holes can "stretch'' supermassive black hole accretion disks

Shuying Zhou, Mouyuan Sun, Tong Liu +3

Stellar black holes (sBHs) are widely believed to exist in the accretion disks of active galactic nuclei (AGNs). Previous studies often focus on the transient emission produced by…

astro-ph.HE2024

How long will the quasar UV/optical flickering be damped?

Shuying Zhou, Mouyuan Sun, Zhen-Yi Cai +3

The UV/optical light curves of Active Galactic Nuclei (AGNs) are commonly described by the Damped Random Walk (DRW) model. However, the physical interpretation of the damping times…

astro-ph.SR2024

The hidden companion in J1527: a 0.69 solar-mass white dwarf?

Zhi-Xiang Zhang, Hao-Bin Liu, Tuan Yi +2

Finding nearby neutron stars can probe the supernova and metal-enrichment histories near our Solar system. Recently, Lin et al. 2023 reported an exciting neutron star candidate, 2M…