Tracing ionized gas kinematics in Lyman-break Analogs Implications for star formation compactness and outflow properties
Context. The ionized gas kinematics of low-mass starburst galaxies is a tracer of galaxy interactions and feedback processes, which are key for understanding massive star formation, chemical enrichment, and galaxy evolution.
| Autores: | , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2026 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:dnet:digitalcsic_::d9f110b4f1fcff9f7253dbdd961813fd |
| Acceso en línea: | http://hdl.handle.net/10261/427510 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxies: ISM Galaxies: kinematics and dynamics Galaxies: starburst |
| Sumario: | Context. The ionized gas kinematics of low-mass starburst galaxies is a tracer of galaxy interactions and feedback processes, which are key for understanding massive star formation, chemical enrichment, and galaxy evolution. |
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