Modeling the origin of the rotation of massive stars
Context. We explore the origins behind the rotation rates of massive stars, accounting for the fact that in contrast to their low-mass siblings, most massive stars do not have detectable magnetic fields. Thus, the star-disk interaction models typically used to simulate the formation of rotating low-...
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| Autori principali: | , , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
EDP Sciences
2026-06-01
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| Serie: | Astronomy & Astrophysics |
| Soggetti: | |
| Accesso online: | https://www.aanda.org/articles/aa/full_html/2026/06/aa58987-26/aa58987-26.html |
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