Chemical diversity of gas in distant galaxies
Overview & Synopsis
The chemical composition of gas in galaxies can be measured in great detail using absorption spectroscopy. By studying gas in galaxies in this way, it is possible to investigate small and faint galaxies, which are the most numerous in the universe. In particular, the chemical distribution of gas in absorbing systems gives us insight into cycles of gas in and around galaxies. In this work we study chemical enrichment within 64 damped Lyman- α absorption systems (DLAs) for redshifts in the range 1.7 < z
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Document Information
| Document Title | Chemical diversity of gas in distant galaxies |
|---|---|
| Author / Organization | T. Ramburuth-Hurt, A. de Cia, J.-K. Krogager, C. Ledoux, P. Petitjean, C. Péroux, M. Dessauges-Zavadsky, J. Fynbo, M. Wendt, Nicolas F. Bouché, C. Konstantopoulou, I. Jermann |
| Subject & Discipline | Multidisciplinary Academic Open Research |
| Categories | Science & Mathematics |
| Publication Year | 2023 |
| License / Rights | Open Access / Creative Commons |
| Resource Verification | Listed PDF (Verification Pending) |
| Original Host Website |
HAL Open Science
(hal.science)
|
| File Format | application/pdf (Portable Document Format) |
| Language | EN |
| Catalog ID | DOC-170871 |
| Original Source Link | Visit Source Page on hal.science » |