A study of pulsation & rotation in a sample of A-K type stars in the <i>Kepler</i> field.

Astrophys Space Sci · 2018 · PMC6280877 · PMID 30595606

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a clear trendno p-value reported

There is a clear trend for hotter stars (especially for ( B − V ) 0 between 0.2 and 0.4) to have shorter rotation periods.

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