Tracing satellite planes in the Sculptor group II. Discovery of five faint dwarf galaxies in the DESI Legacy Survey
Context. Although substantial progress has been made in reconciling lambda cold dark matter (ΛCDM) simulations with the observed abundance and distribution of satellite galaxies, important tensions persist. Studying satellite systems around spiral galaxies thus remains key to addressing these tensio...
| 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_::f22239fb1079e08f683c96942949158e |
| Acceso en línea: | http://hdl.handle.net/10261/428646 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxies: dwarf Galaxies: individual: NGC 253 Galaxies: structure Dark matter |
| Sumario: | Context. Although substantial progress has been made in reconciling lambda cold dark matter (ΛCDM) simulations with the observed abundance and distribution of satellite galaxies, important tensions persist. Studying satellite systems around spiral galaxies thus remains key to addressing these tensions. |
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