activity
20242026
most citedTentative Detection of the Glycine Isomer Glycolamide in Hot Molecular Core

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

collaborators

7 papers

astro-ph.GA2026

Molecule-dependent Abundance Behavior of Oxygen-bearing Complex Organics in High-Mass Star-Forming Regions: A Uniform 50-source Survey

Xuefang Xu, Mingwei He, Qian Gou +10

We present a uniform IRAM-30\,m survey analysis of four oxygen-bearing complex organic molecules (COMs), methanol (CHOH), acetaldehyde (CHCHO), methyl formate (CHOCHO),…

astro-ph.GA2026

First Interstellar Detection of Methyl Carbamate: A New Observational Anchor for Glycine Chemistry

Chunguo Duan, Fengwei Xu, Jun Kang +5

Glycine-the simplest amino acid-has remained undetected in the interstellar medium despite decades of sensitive searches, motivating alternative approaches to constrain its astroch…

astro-ph.GA20261 cited

Tentative Detection of the Glycine Isomer Glycolamide in Hot Molecular Core

Chunguo Duan, Fengwei Xu, Qian Gou +6

Understanding whether prebiotic molecules can endure and reform through the energetic stages of star formation is essential for tracing the continuity of interstellar chemistry tow…

astro-ph.GA2025

The ALMA-QUARKS survey: Extensive detection of acetamide in multiple high-mass star-forming regions

Chunguo Duan, Xuefang Xu, Qian Gou +8

Acetamide (CHCONH), a key interstellar amide and a methyl derivative of formamide (NHCHO), has been sparsely detected, limiting insights into its prebiotic releva…

astro-ph.GA2025

An ALMA Study of Molecular Complexity in the Hot Core G336.99-00.03 MM1

Chunguo Duan, Qian Gou, Tie Liu +9

High-mass star formation involves complex processes, with the hot core phase playing a crucial role in chemical enrichment and the formation of complex organic molecules. However,…

astro-ph.SR2024

3 mm Spectroscopic Observations of Massive Star-Forming Regions with IRAM 30-m

Xuefang Xu, Junzhi Wang, Qian Gou +6

Broadband spectroscopic observations with high sensitivity provide an unbiased way to detect emissions of molecules in space. We present deep observations from ~ 105.8 GHz to 113.6…