activity
20032026
most citedHierarchical fragmentation and differential star formation in the Galactic "Snake": infrared dark cloud G11.11-0.12

264 citations · 2.9k across the 99 of their papers we have counts for

collaborators

99 papers

astro-ph.GA2026

The Epoch of the GSE Merger: Insights from the Splash and Thick Disk Age Distributions

Sihan Lu, Yang Huang, Qikang Feng +1

The epoch of the Gaia-Sausage-Enceladus (GSE) merger, the last major merger experienced by the Milky Way, is crucial for reconstructing the Galaxy's evolutionary history. This even…

astro-ph.SR2026

A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to dex. II. Lithium Abundance and New Insight to the Lithium Plateau

Hong-Liang Yan, Jinxiao Qin, Shuai Liu +12

Metal-poor stars are crucially important for understanding the early Galaxy, first stars, and the Universe. In this series of papers, we present a homogeneous non-local thermodynam…

astro-ph.GA2026

An Old, Low-mass, Metal-poor Hypervelocity Star Candidate Consistent with a Galactic Center Origin

Shunhong Deng, Yang Huang, Haozhu Fu +4

We report the discovery of DESI-HVS1, a hypervelocity star (HVS) candidate identified from DESI DR1 spectroscopy and Gaia DR3 astrometry. DESI-HVS1 is an old, low-mass, metal-poor…

astro-ph.GA2026

The Fate of the Milky Way--Andromeda System: To Merge or Not?

Hao Wu, Yang Huang, Huawei Zhang +2

It has long been predicted that the Milky Way (MW) will eventually merge with Andromeda (M31), a view reinforced by \textit{HST} measurements indicating a small M31 transverse velo…

astro-ph.HE2026

Spectral Dataset of Stripped-Envelope Supernovae from the Tsinghua Supernova Group

Danfeng Xiang, Xiaofeng Wang, Jujia Zhang +40

The extent of envelope stripping in the progenitor stars is directly reflected in the diversity of spectral features observed in stripped-envelope supernovae (SESNe). Through exten…

astro-ph.GA2025

The rotation curve of the Milky Way measured by Classical Cepheids from Gaia DR3

Qikang Feng, Yang Huang, Huawei Zhang +1

We determine the rotation curve (RC) of the Milky Way in the range 6 < R < 18 kpc using a sample of 903 carefully selected classical Cepheids with precise proper motions and high-q…