activity
20242026
most citedStellar feedback drives the baryon deficiency in low-mass galaxies

1 citations · 1 across the 3 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2026

Warped Disk Galaxies: Alignment with the Large-Scale Tidal Field

Yiheng Wang, Huiyuan Wang, Enci Wang +1

A possible origin of disk galaxy warps is the misalignment between galactic disks and their host dark matter halos, the orientations of which are found to be statistically aligned…

astro-ph.GA20261 cited

Stellar feedback drives the baryon deficiency in low-mass galaxies

Haoran Yu, Enci Wang, Zeyu Chen +8

Stellar feedback, as a key process regulating the baryon cycle, is thought to greatly redistribute baryonic material inside and outside the dark matter halos (DMHs), however the ob…

astro-ph.GA2026

A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications

Yuan Wang, Xiong Luo, Huiyuan Wang +5

Precession is a very common phenomenon for small-scale astronomical objects. However, the precession of galactic disks, occurring on a scale larger than kilo-parsec, has barely bee…

astro-ph.GA2026

Symmetry in Fundamental Parameters of Galaxies on the Star-forming Main Sequence

Zhicheng He, Enci Wang, Luis C. Ho +4

The Star-Forming Main Sequence (SFMS) serves as a critical framework for understanding galaxy evolution, highlighting the relationship between star formation rates (SFR) and stella…

astro-ph.GA2026

The First Systematic Survey of Stellar Halos in High-Inclination Galaxies Reveals Unusually Quiescent Merger Histories of Nearby Galaxies

Bojun Tao, Hong-Xin Zhang, Wenting Wang +8

Stellar halos are the only major stellar component of disk galaxies that lack systematic observational characterization, yet they encode critical information about galaxy merger hi…

astro-ph.GA2026

Updated Metallicity Diagnostics for Precision Oxygen Abundance Measurements in High-redshift Galaxies with JWST

Shihong Liu, Yu Rong, Tie Li +7

Recent work has demonstrated that widely used strong-line oxygen abundance indicators, such as O3N2, , and , suffer from large uncertainties when applied…