Spiral arms across stellar populations in simulations via the local dimension method
[Context] The origin and nature of spiral arms remain unclear. Star forming regions and young stars are generally strongly associated to the spiral structure, but there are few quantitative predictions from simulations about the involvement of stars of different ages.
| Autores: | , , , , , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2026 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:dnet:digitalcsic_::ad0375fa9d29daaeacf3c94556e8ae05 |
| Acesso em linha: | http://hdl.handle.net/10261/426002 http://arxiv.org/abs/2507.15473v1 |
| Access Level: | acceso abierto |
| Palavra-chave: | Galaxies: spiral Galaxies: stellar content Galaxies: structure Galaxy: disk Galaxy: stellar content Galaxy: structure |
| Resumo: | [Context] The origin and nature of spiral arms remain unclear. Star forming regions and young stars are generally strongly associated to the spiral structure, but there are few quantitative predictions from simulations about the involvement of stars of different ages. |
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