PIMMS extends ZDI by adding a pulsation velocity map to reconstruct surface brightness, magnetic field, and velocity from spectropolarimetric data, with numerical tests showing accurate recovery on simulated pulsating hot stars.
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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.
citing papers explorer
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PIMMS: Pulsation-Informed Magnetic Mapping of Stars with Zeeman-Doppler Imaging I. Formalism and numerical tests
PIMMS extends ZDI by adding a pulsation velocity map to reconstruct surface brightness, magnetic field, and velocity from spectropolarimetric data, with numerical tests showing accurate recovery on simulated pulsating hot stars.
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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.