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Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds
Document de travail - Pré-publication -
The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky Way
Document de travail - Pré-publication -
Physical conditions in the gas phases of the giant HII region LMC-N11: II. Origin of [CII] and fraction of CO-dark gas
Document de travail - Pré-publication