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Prof. Dr. Maria N. Drozdovskaya, Department of Chemistry, Biochemistry, and Pharmaceutical Sciences, University of Bern
Photo Credit: © University of Bern, Image: Vera Knöpfel
Scientific Frontline: Extended "At a Glance" Summary: Interstellar Methanol in Protostellar Systems
The Core Concept: Complex organic molecules, specifically standard and fully deuterated methanol, are forming within the dense gas and dust clouds surrounding young, low-mass protostars.
Key Distinction/Mechanism: Unlike previous observations that limited methanol maser emissions strictly to high-mass protostars, recent data reveals these emissions are abundant around low-mass, Sun-like stars, indicating that locally extreme physical conditions also prevail in these early environments.
Origin/History: The discoveries were published in 2026 by the international COMPASS (Complex Organic Molecules in Protostars with ALMA Spectral Surveys) project, which utilized the Atacama Large Millimeter/submillimeter Array (ALMA) to study the chemical composition of eleven nearby protostars.
Major Frameworks/Components:
- The detection of methanol maser emissions, which act as distinctive radio signals, in the precursors of relatively light, Sun-like stars.
- The first-ever interstellar discovery of fully deuterated methanol (CD₃OD), a rare variant where all hydrogen atoms are replaced by the heavy isotope deuterium, surrounding the protostar IRAS 4A2 in the Perseus molecular cloud.
- The use of high-performance spectroscopic measurements to analyze the transfer of chemical diversity from molecular clouds to planetary systems.



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