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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Enhanced mass transfer events trigger the nova eruptions in T CrB by building 95% of the ignition envelope mass on a 1.29 solar-mass white dwarf via a high-viscosity disk.
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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The accretion-driven eruption of the recurrent nova T Corona Borealis
Enhanced mass transfer events trigger the nova eruptions in T CrB by building 95% of the ignition envelope mass on a 1.29 solar-mass white dwarf via a high-viscosity disk.