Gas excitation of post-SB galaxies at 0.6 < z < 1.3
Context. Molecular gas in galaxies traces both the fuel for star formation and the processes that enhance or suppress it. Observing its physical state (e.g., excitation) can reveal when and why galaxies stop forming stars. Aims. We observed the CO(5–4) emission of eight post-SB galaxies at z ∼ 0.6 −...
| Published in: | Astronomy & Astrophysics |
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| Main Authors: | , , , |
| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2026-05-01
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| Subjects: | |
| Online Access: | https://www.aanda.org/articles/aa/full_html/2026/05/aa58073-25/aa58073-25.html |