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Astronomy & Astrophysics 689 A64 (2024)
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Observed CN and HCN intensity ratios exhibit subtle variations in extreme galaxy environments

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LEGO – II. A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions within the Milky Way disc

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Spectropolarimetry of the superwind filaments of the starburst galaxy M 82 II: Kinematics of the dust surrounding the nuclear starburst

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Exploring the CO/CN line ratio in nearby galaxies with the ALMA archive

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AFTER THE INTERACTION: AN EFFICIENTLY STAR-FORMING MOLECULAR DISK IN NGC 5195

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