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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 -
GLOSTAR -- Radio Source Catalog II: $28^\circ < \ell < 36^\circ$ and $|b| < 1^\circ$, VLA B-configuration
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 -
On the similarity of IR-bright and IR-dark molecular clouds
(2014-06-12)Document de travail - Pré-publication