Tomography of the red supergiant star {μ} Cep
classification
🌌 astro-ph.SR
keywords
starsupergiantaimingappliedatmospheresatmosphericconstraindepth
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A tomographic method, aiming at probing velocity fields at depth in stellar atmospheres, is applied to the red supergiant star {\mu} Cep and to snapshots of 3D radiative-hydrodynamics simulation in order to constrain atmospheric motions and relate them to photometric variability.
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