Low-mass companions and higher viscosity suppress Kozai-Lidov oscillations and disc tearing in Be star disc models, while radiative transfer predicts a first-ever triple-peaked H-alpha line from the oscillating disc.
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Investigating Kozai-Lidov Oscillations and Disc Tearing in Be Star Discs
Low-mass companions and higher viscosity suppress Kozai-Lidov oscillations and disc tearing in Be star disc models, while radiative transfer predicts a first-ever triple-peaked H-alpha line from the oscillating disc.