Ensemble pulsational characteristics of eclipsing binaries containing beta Cep stars observed by the TESS mission

arXiv:2610.01679 · astro-ph.SR · Submitted 2026-10-01 · Read on arXiv

astro-ph.SR

Submitted: 2026-10-01

Updated: 2026-10-01

Terminology

• Core — 19× in this paper · explained in 2 episodes
• Angular Momentum Transport — 2× in this paper · explained in 3 episodes
• European Research Council — 2× in this paper
• Alignment — 1× in this paper · explained in 1 episode
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Bayesian Information Criterion — 1× in this paper
• Metallicity — 1× in this paper · explained in 3 episodes
• Mikulski Archive for Space Telescopes — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes
• Verification — 1× in this paper · explained in 2 episodes

Sources

• Oscillation Frequencies of Moderately Rotating Delta Scuti Stars: Asymmetric Mode Splittings Due to Non-spherical Distortion
• Localizing Sources of Variability in Crowded TESS Photometry
• Pulsations in Binary Star Systems

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