activity
20242026
collaborators

6 papers

astro-ph.GA2026

Post-starburst Galaxies with Active Galactic Nucleus: Properties and Evolutionary Sequences

Junjie Huang, Yanmei Chen, Yong Shi +7

Post-starburst (PSB) galaxies, identified by strong Balmer absorption and weak nebular emission, provide a key laboratory for studying rapid quenching. Using the final data release…

astro-ph.GA2026

Properties of Galaxies with Counter-rotating Stellar Disks in the MaNGA Survey

Min Bao, Zhenyu Tang, Yanmei Chen +2

Gas accretion process can fuel both star formation and black hole activity, playing a critical role in galaxy evolution. The counter-rotating structures are believed to originate f…

astro-ph.GA2025

Clumpy Starburst in a Local Dwarf Galaxy, NGC 1522

Liuze Long, Yulong Gao, Qiusheng Gu +8

To investigate the star-forming process in nearby dwarf galaxies, we present Integral Field Units (IFU) observation of the star-forming dwarf galaxy, NGC 1522, with the Very Large…

astro-ph.GA2025

A Dual Active Black Hole Candidate with Mass Ratio ~7:1 in a Disk Galaxy

Xiao Cao, Yan-Mei Chen, Yong Shi +8

Dual active galactic nuclei (AGNs) with comparable masses are commonly witnessed among the major merged galaxies with interaction remnants. Considering almost every massive galaxy…

astro-ph.GA2024

PGC 44685: A Dwarf Star-forming Lenticular Galaxy with Wolf-Rayet Population

Shiying Lu, Qiusheng Gu, Yulong Gao +8

Lenticular galaxies (S0s) are formed mainly from the gas stripping of spirals in the cluster. But how S0s form and evolve in the field is still untangled. Based on spatially resolv…

astro-ph.GA2024

Quasars with Flare/Eclipse-like Variability Identified in ZTF

Zhiyuan Zheng, Yong Shi, Shuowen Jin +4

Active galactic nuclei (AGNs) are known to exhibit optical/UV variability and most of them can be well modeled by the damped random walks. Physical processes that are not related t…