First identification of a stationary l=3 sectoral pulsation mode in any delta Scuti star, appearing as frequencies split by precisely 6 times the orbital frequency due to binary perturbations.
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MESA Star has been substantially updated with new capabilities for low-mass giant planets, asteroseismology coupling, rotating star models, and uninterrupted massive star evolution to core collapse.
citing papers explorer
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Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode
First identification of a stationary l=3 sectoral pulsation mode in any delta Scuti star, appearing as frequencies split by precisely 6 times the orbital frequency due to binary perturbations.
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Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
MESA Star has been substantially updated with new capabilities for low-mass giant planets, asteroseismology coupling, rotating star models, and uninterrupted massive star evolution to core collapse.