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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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
A new sample of young candidate Bridge stars is identified and shown to align with gas structures, with kinematics implying a ~125 Myr crossing time consistent with the last LMC-SMC interaction.
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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Characterisation of the Clouds' young stellar Bridge using Gaia DR3
A new sample of young candidate Bridge stars is identified and shown to align with gas structures, with kinematics implying a ~125 Myr crossing time consistent with the last LMC-SMC interaction.