A small subset of long secondary period stars shows relative harmonic phases consistent with highly inclined oscillatory convective dipole modes rather than binary systems.
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Tayler-Spruit magnetic fields can convert low-frequency internal gravity waves to magneto-gravity waves in low-mass star cores, with effects strongest on the red giant branch in central regions.
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Harmonic phase diagnostics of long secondary periods. Testing predictions of oscillatory convective dipole modes in the OGLE sample
A small subset of long secondary period stars shows relative harmonic phases consistent with highly inclined oscillatory convective dipole modes rather than binary systems.
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Co-existence of Internal Gravity Waves and Tayler-Spruit Magnetic Fields in the Radiative Core of Low-mass Stars
Tayler-Spruit magnetic fields can convert low-frequency internal gravity waves to magneto-gravity waves in low-mass star cores, with effects strongest on the red giant branch in central regions.