Physical conditions of the molecular gas in metal-poor galaxies
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DOI: 10.1051/0004-6361/201731000
Abstract: Studying the molecular component of the interstellar medium (ISM) in metal-poor galaxies has been challenging because of the faintness of carbon monoxide emission, the most common proxy of H2. Here we present new detections of… read more here.
Keywords: metal poor; physical conditions; molecular gas; gas ... See more keywords