Mocking integral field unit observations and metallicity diagnostics from cosmological simulations
Context. Hydrodynamic simulations are powerful tools for studying galaxy formation. However, it is crucial to test and improve the subgrid physics underlying these simulations by comparing their predictions with observations. To this aim, observable quantities can be derived for simulated galaxies,...
| Autores: | , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/397946 |
| Acceso en línea: | http://hdl.handle.net/10261/397946 |
| Access Level: | acceso abierto |
| Palabra clave: | ISM: abundances Dust, extinction HII regions Galaxies: ISM Galaxies: star formation |
| Sumario: | Context. Hydrodynamic simulations are powerful tools for studying galaxy formation. However, it is crucial to test and improve the subgrid physics underlying these simulations by comparing their predictions with observations. To this aim, observable quantities can be derived for simulated galaxies, enabling the analysis of simulated properties through an observational approach. |
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