activity
20232026
most citedThe robustness in identifying and quantifying high-redshift bars using JWST observations

16 citations · 44 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

FAST Observations of Filamentary and Compact H I Structure in a Magellanic Stream IV Field

Yuxin Xiao, Qingzheng Yu, Taotao Fang +3

The Magellanic Stream (MS) is believed to have formed from gas removed from the Large and Small Magellanic Clouds through tidal forces and hydrodynamic interactions with the Milky…

astro-ph.GA2026

The Intrinsic Multiphase Gas--Black Hole Connection across Scales in IllustrisTNG

Xiaoxia Zhang, Taotao Fang, Shulan Yan +2

The relationship between supermassive black holes and the multiphase circumgalactic medium is central to understanding the co-evolution of galaxies and their central black holes. W…

astro-ph.GA2026

Environmental Imprints on the Assembly of the Cool Gas around Bright Cluster Galaxies

Runyu Zhu, Hu Zou, Taotao Fang +14

Galaxy clusters represent extreme cosmic laboratories where environmental processes dramatically reshape their constituent galaxies, yet their effect on the gaseous halos of centra…

astro-ph.HE2026

Thermal emission from dark matter-heated neutron stars in the Galactic Center

Yunhe Hu, Feng Huang, Taotao Fang

We investigate the thermal impact of dark matter (DM) capture and annihilation on neutron stars (NSs) in the Galactic Center (GC). Accounting for both kinetic energy deposition and…

astro-ph.GA2026★ 2 cited

The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk

Xiaochuan Jiang, Taotao Fang, Shulan Yan

The physical properties of Milky Way Mgii-bearing gas remain poorly constrained due to the saturation of the near-UV doublet. We utilize the weaker Mgii 1239, 1240 doublet from…

astro-ph.GA2026

COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 m Since

Si-Yue Yu, Andreas L. Faisst, Taotao Fang +7

We present the evolution of galaxy size and surface brightness in the rest-frame band (1.22 m), tracing the stellar mass distribution, over , using a samp…