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- W4300857599 abstract "Context. The early stage of stellar evolution is characterized by a magnetic coupling between a star and its accretion disc, known as a star-disc locking mechanism. The disc-locking prevents the star to spin its rotation up, and its timescale depends on the disc lifetime, which should not be longer than about 10 Myr. Some mechanisms can significantly shorten this lifetime, allowing a few stars to start spinning up much earlier than other stars and increasing the observed rotation period dispersion among coeval stars." @default.
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- W4300857599 date "2014-10-01" @default.
- W4300857599 modified "2023-09-28" @default.
- W4300857599 title "Evidence from stellar rotation of enhanced disc dispersal" @default.
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- W4300857599 doi "https://doi.org/10.1051/0004-6361/201423832" @default.
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