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The Interior Angular Momentum of Core Hydrogen Burning Stars from Gravity-mode Oscillations
2017
Astrophysical Journal Letters
A major uncertainty in the theory of stellar evolution is the angular momentum distribution inside stars and its change during stellar life. We compose a sample of 67 stars in the core-hydrogen burning phase with a g value from high-resolution spectroscopy, as well as an asteroseismic estimate of the near-core rotation rate derived from gravity-mode oscillations detected in space photometry. This assembly includes 8 B-type stars and 59 AF-type stars, covering a mass range from 1.4 to 5 M_,
doi:10.3847/2041-8213/aa8a62
fatcat:ttetcueorzf3lbkazaxg6lag44