PHANGS-MeerKAT and MHONGOOSE HI observations of nearby spiral galaxies: Physical drivers of the molecular gas fraction, R mol
The molecular-to-atomic gas ratio is crucial to our understanding of the evolution of the interstellar medium (ISM) in galaxies. We investigated the balance between the atomic (Σ HI ) and molecular gas (Σ H2 ) surface densities in eight nearby star-forming galaxies using new high-quality observation...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2024-11, Vol.691, p.A163 |
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Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
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