Magnetohydrodynamic simulations of A-type stars: Long-term evolution of core dynamo cycles
[Context] Early-type stars have convective cores due to a steep temperature gradient produced by the CNO cycle. These cores can host dynamos and the generated magnetic fields may be relevant in explaining the magnetism observed in Ap/Bp stars.
| Authors: | , , , , |
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| Format: | article |
| Status: | Published version |
| Publication Date: | 2024 |
| Country: | España |
| Institution: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repository: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/384096 |
| Online Access: | http://hdl.handle.net/10261/384096 http://arxiv.org/abs/2409.18066v1 |
| Access Level: | Open access |
| Keyword: | Dynamo Magnetic fields Magnetohydrodynamics (MHD) Stars: chemically peculiar Stars: early-type Stars: magnetic field |
| Summary: | [Context] Early-type stars have convective cores due to a steep temperature gradient produced by the CNO cycle. These cores can host dynamos and the generated magnetic fields may be relevant in explaining the magnetism observed in Ap/Bp stars. |
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