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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Principais autores:	Oliva André, Moyano Facundo D., Sciarini Luca, Ekström Sylvia, Eggenberger Patrick, Meynet Georges
Format:	Artigo
Jezik:	Inglês
Izdano:	EDP Sciences 2026-06-01
Serija:	Astronomy & Astrophysics
Teme:	stars: formation stars: massive stars: pre-main sequence stars: rotation ism: jets and outflows
Online dostop:	https://www.aanda.org/articles/aa/full_html/2026/06/aa58987-26/aa58987-26.html
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