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20242026
most citedA negative stellar massgaseous metallicity gradient relation of dwarf galaxies modulated by stellar feedback

6 citations · 14 across the 7 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

Evidence for the transformation from lenticular to spiral galaxies

Mengkui Zhou, Huiyuan Wang, Ran Li +8

It is widely accepted that late-type galaxies, such as spirals, evolve into early-type systems, including elliptical and lenticular galaxies, through galaxy mergers and violent dis…

astro-ph.GA2025

The Internal Kinematics, Stellar Population, and Gas-phase Properties of The Pseudobulge in An Ultra-diffuse Galaxy: AGC721966

Shihong Liu, Yu Rong, Huiyuan Wang +8

Leveraging spectroscopic data from the Sloan Digital Sky Survey, we conduct a comprehensive analysis of the central stellar velocity dispersion, stellar population properties, star…

astro-ph.GA2025★ 6 cited

A negative stellar massgaseous metallicity gradient relation of dwarf galaxies modulated by stellar feedback

Tie Li, Hong-Xin Zhang, Wenhe Lyu +16

Baryonic cycling is reflected in the spatial distribution of metallicity within galaxies, yet gas-phase metallicity distribution and its connection with other properties of dwarf g…

astro-ph.GA2024

Ultra Diffuse Dwarf Galaxies Hosting Pseudo-bulges

Yu Rong, Hong-Xin Zhang, Cheng Cheng +5

By analyzing data from DESI Legacy Imaging Survey of the dwarf galaxies in the Arecibo Legacy Fast Alfa Survey, we have identified five ultra-diffuse galaxies (UDGs) featuring cent…

astro-ph.GA2024

Intrinsic Morphology of The Stellar Components in HI-bearing Dwarf Galaxies and The Dependence on Mass

Yu Rong, Min He, Huijie Hu +2

The intrinsic morphology of stellar components within HI-bearing dwarf galaxies remains a topic of uncertainty. Leveraging the galaxy dataset derived from the cross-matched catalog…

astro-ph.GA2024★ 3 cited

Gas-rich Ultra-diffuse Galaxies Are Originated from High Specific Angular Momentum

Yu Rong, Huijie Hu, Min He +5

Ultra-diffuse galaxies, characterized by comparable effective radii to the Milky Way but possessing 100-1,000 times fewer stars, offer a unique opportunity to garner novel insights…