Ko-Ju Chuang

Assistant prof.

Leiden University

Netherlands

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Ko-Ju Chuang is an Assistant Professor at Leiden University in the Netherlands. His research focuses on interstellar chemistry, including the formation and reactivity of complex organic molecules in various astrophysical environments. Recent articles by Dr. Chuang explore topics such as laboratory infrared spectra of carbonyl sulfide and the role of ammonium hydrosulfide in interstellar ices.

Articles (19)

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2025

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2025

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2022

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2022

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2020

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2020

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2020

Collaborators (6)

Herma M. Cuppen

Radboud University

NETHERLANDS

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Patrick Kavanagh

Assistant Professor

National University of Ireland, Maynooth

IRELAND

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Thanja Lamberts

Leiden University

NETHERLANDS

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Sergio Ioppolo

Aarhus University

DENMARK

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Harold Linnartz

NETHERLANDS

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Julia C. Santos

Leiden University

NETHERLANDS

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Ko-Ju Chuang

Research Interests

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About

Articles (19)

Laboratory Infrared Spectra and Band Strengths of Carbonyl Sulfide (OCS) in CH3OH- and CO-Rich Ice Mixtures for Analyzing Interstellar Ice Observations

Ammonium hydrosulfide (NH4SH) as a potentially significant sulfur sink in interstellar ices

Production of linear alkanes via the solid-state hydrogenation of interstellar polyynes

Formation of S-Bearing Complex Organic Molecules in Interstellar Clouds via Ice Reactions with C2H2, HS, and Atomic H

Formation of N–bearing complex organic molecules in molecular clouds: Ketenimine, acetonitrile, acetaldimine, and vinylamine via the UV photolysis of C2H2 ice

Pulsed ion deflection to overcome detector saturation in cryogenic ice sampling

Spatially resolving the volatile sulfur abundance in the HD 100546 protoplanetary disc

Formation of carbonyl sulfide (OCS) via SH radicals in interstellar CO-rich ice under dense cloud conditions

The hunt for formamide in interstellar ices

Interstellar Carbonaceous Dust Erosion Induced by X-Ray Irradiation of Water Ice in Star-forming Regions

First Experimental Confirmation of the CH3O + H2CO → CH3OH + HCO Reaction: Expanding the CH3OH Formation Mechanism in Interstellar Ices

Formation of the Simplest Amide in Molecular Clouds: Formamide (NH2CHO) and Its Derivatives in H2O-rich and CO-rich Interstellar Ice Analogs upon VUV Irradiation

Methane Formation in Cold Regions from Carbon Atoms and Molecular Hydrogen

Methoxymethanol formation starting from CO hydrogenation

Hydrogenation of Accreting C Atoms and CO Molecules–Simulating Ketene and Acetaldehyde Formation Under Dark and Translucent Cloud Conditions

Formation of complex organic molecules in molecular clouds: acetaldehyde, vinyl alcohol, ketene, and ethanol via the “energetic” processing of C2H2 ice

A non-energetic mechanism for glycine formation in the interstellar medium

A cryogenic ice setup to simulate carbon atom reactions in interstellar ices

An experimental study of the surface formation of methane in interstellar molecular clouds

Collaborators (6)

Herma M. Cuppen

Patrick Kavanagh

Thanja Lamberts

Sergio Ioppolo

Harold Linnartz

Julia C. Santos

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