Radial differential rotation leading to dipole collapse in pre-main-sequence stars
Context. Despite significant progress in the observational characterization of stellar magnetic fields, the physical processes that govern their intensity and topology, which could certainly result from their formation history, remain poorly understood. During the pre-main-sequence (PMS) phase, the...
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| Hauptverfasser: | , , , |
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| Format: | Artigo |
| Sprache: | Inglês |
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EDP Sciences
2026-03-01
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| Schriftenreihe: | Astronomy & Astrophysics |
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| Online-Zugang: | https://www.aanda.org/articles/aa/full_html/2026/03/aa57616-25/aa57616-25.html |
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