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W2551556093 abstract "Context. Constraints on the internal rotation of red giants are now available thanks to asteroseismic observations. Preliminary comparisons with rotating stellar models indicate that an undetermined additional process for the internal transport of angular momentum is required in addition to purely hydrodynamic processes." @default.
W2551556093 created "2016-11-30" @default.
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W2551556093 date "2017-02-21" @default.
W2551556093 modified "2023-10-02" @default.
W2551556093 title "Constraining the efficiency of angular momentum transport with asteroseismology of red giants: the effect of stellar mass" @default.
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W2551556093 doi "https://doi.org/10.1051/0004-6361/201629459" @default.
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