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G331.512โ0.103: An Interstellar Laboratory for Molecular Synthesis. I. The Ortho-to-para Ratios for CH<sub>3</sub>OH and CH<sub>3</sub>CN
Abstract Spectral line surveys reveal rich molecular reservoirs in G331.512โ0.103, a compact radio source in the center of an energetic molecular outflow. In this first work, we analyze the physical conditions of the source by means of CH 3 OH and CH 3 CN. The observations were performed with the โฆ