Protostellar spin-up and fast rotator formation through binary star formation
Protostellar spin-up and fast rotator formation through binary star formation
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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(Edited) Many fast rotator stars (rotation periods of < 2 days) are found in unresolved binaries with separations of tens of au. This correlation leads to the question of whether the formation of binary stars inherently produces fast rotators. We aim to understand whether the formation of companions plays a role in spinning up stars. We use magneto...
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Protostellar spin-up and fast rotator formation through binary star formation
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TN_cdi_proquest_journals_3044055470
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3044055470
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2404.14210
