A PSF-fitting pipeline extracts variability light curves for 91 SMC massive stars and finds that stochastic low-frequency variability morphology tracks HR-diagram position independently of metallicity.
2008.11162
2 Pith papers cite this work. Polarity classification is still indexing.
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Overview of asteroseismology principles, data needs, forward modeling methods, key results across the HR diagram, and future challenges.
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Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images
A PSF-fitting pipeline extracts variability light curves for 91 SMC massive stars and finds that stochastic low-frequency variability morphology tracks HR-diagram position independently of metallicity.
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Asteroseismology
Overview of asteroseismology principles, data needs, forward modeling methods, key results across the HR diagram, and future challenges.