papers

Publications (10)

astro-ph.CO2012

Clumpy accretion onto black holes. I. Clumpy-ADAF structure and radiation

J. -M. Wang, C. Cheng, Y. -R. Li

In this paper, we investigate the dynamics of clumps embedded in and confined by the advection-dominated accretion flows (ADAF), in which collisions among the clumps are neglected.…

astro-ph.CO2010

Accretion Disks in Active Galactic Nuclei: Gas Supply Driven by Star Formation

J. -M. Wang, C. -S. Yan, H. -Q. Gao +3

Self-gravitating accretion disks collapse to star-forming(SF) regions extending to the inner edge of the dusty torus in active galactic nuclei (AGNs). A full set of equations inclu…

astro-ph.HE2023

Accretion-modified Stars in Accretion Disks of Active Galactic Nuclei: the Low-luminosity Cases and an Application to Sgr A

J. -M. Wang, J. -R. Liu, Y. -R. Li +3

In this paper, we investigate the astrophysical processes of stellar-mass black holes (sMBHs) embedded in advection-dominated accretion flows (ADAFs) of supermassive black holes (S…

astro-ph.GA2023

Star Formation in Self-gravitating Disks in Active Galactic Nuclei. III. Efficient Production of Iron and Infrared Spectral Energy Distributions

J. -M. Wang, S., Zhai +7

Strong iron lines are a common feature of the optical spectra of active galactic nuclei (AGNs) and quasars from to the local Universe, and [Fe/Mg] ratios do not show co…

astro-ph.GA2020

Dynamical evidence of the sub-parsec counter-rotating disc for a close binary of supermassive black holes in the nucleus of NGC 1068

J. -M. Wang, Y. -Y. Songsheng, Y. -R. Li +2

It arises a puzzle in \NGC\, how to secularly maintain the counter-rotating disc from to pc unambiguously detected by recent ALMA observations of molecular gas. Upon fur…

astro-ph.GA2011

Star formation in self-gravitating disks in active galactic nuclei. I. Metallicity gradients in broad line regions

J. -M. Wang, J. -Q. Ge, C. Hu +6

It has been suggested that the high metallicity generally observed in active galactic nuclei (AGNs) and quasars originates from ongoing star formation in the self-gravitating part…

astro-ph.CO2013

Supermassive black holes with high accretion rates in active galactic nuclei: I. First results from a new reverberation mapping campaign

P. Du, C. Hu, K. -X. Lu +7

We report first results from a large project to measure black hole (BH) mass in high accretion rate active galactic nuclei (AGNs). Such objects may be different from other AGNs in…

astro-ph.GA2022

Spiral Arms in Broad-line Regions of Active Galactic Nuclei. I. Reverberation and Differential Interferometric Signals of Tightly Wound Cases

J. -M. Wang, P. Du, Y. -Y. Songsheng +1

As a major feature in spectra of active galactic nuclei, broad emission lines deliver information of kinematics and spatial distributions of ionized gas surrounding the central sup…

astro-ph.GA2023

Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XIII. Ultraviolet Time Lag of H Emission in Mrk 142

V. C. Khatu, S. C. Gallagher, K. Horne +17

We performed a rigorous reverberation-mapping analysis of the broad-line region (BLR) in a highly accreting () active galactic nucleus, Markarian 142 (…

astro-ph.GA2009

Episodic Random Accretion and the Cosmological Evolution of Supermassive Black Hole Spins

J. -M. Wang, C. Hu, Y. -R. Li +7

The growth of supermassive black holes (BHs) located at the centers of their host galaxies comes mainly from accretion of gas, but how to fuel them remains an outstanding unsolved…