Shaping core dynamos in A-type stars: The role of dipolar fossil fields
[Context] Large-scale magnetic fields of Ap/Bp stars are stable over long timescales and typically have simple dipolar geometries, leading to the idea of a fossil origin. These stars are also expected to have convective cores that can host strong dynamo action.
| Autores: | , , , , |
|---|---|
| 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:10261/398694 |
| Acceso en línea: | http://hdl.handle.net/10261/398694 http://arxiv.org/abs/2506.01017v1 |
| Access Level: | acceso abierto |
| Palabra clave: | Dynamo Magnetohydrodynamics (MHD) Stars: early-type Stars: magnetic field |
| Sumario: | [Context] Large-scale magnetic fields of Ap/Bp stars are stable over long timescales and typically have simple dipolar geometries, leading to the idea of a fossil origin. These stars are also expected to have convective cores that can host strong dynamo action. |
|---|