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ChronoFlow: A Data-driven Model for Gyrochronology

Gyrochronology is a technique for constraining stellar ages using rotation periods, which change over a star’s main-sequence (MS) lifetime due to magnetic braking. This technique shows promise for MS FGKM stars, where other methods are imprecise. However, the observed dispersion in rotation rates fo...

Täydet tiedot

Tallennettuna:
Päätekijät: Phil R. Van-Lane, Joshua S. Speagle, Gwendolyn M. Eadie, Stephanie T. Douglas, Phillip A. Cargile, Catherine Zucker, Yuxi (Lucy) Lu, Ruth Angus
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2025-01-01
Sarja:The Astrophysical Journal
Aiheet:
Open star clusters
Stellar rotation
Stellar ages
Dwarf stars
Main sequence stars
Astrostatistics
Linkit:https://doi.org/10.3847/1538-4357/adcd73
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