Interferometric time series show steady mass loss in Miras tied to large-amplitude fundamental-mode pulsations, while RSGs like VX Sgr undergo extreme mass-loss events linked to pulsation mode changes and shocks.
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A small subset of long secondary period stars shows relative harmonic phases consistent with highly inclined oscillatory convective dipole modes rather than binary systems.
citing papers explorer
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VLTI-GRAVITY measurements of cool evolved stars: II. Pulsation properties and mass-loss process of the Mira star R Car and the red supergiant VX Sgr
Interferometric time series show steady mass loss in Miras tied to large-amplitude fundamental-mode pulsations, while RSGs like VX Sgr undergo extreme mass-loss events linked to pulsation mode changes and shocks.
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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.