Rot. distributions from TESS-APOGEE-Kepler-Gaia
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https://b2find.eudat.eu/dataset/e927b4d9-5586-5dfc-a13c-8c5cbcb737fa
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Stellar rotation is a complex function of mass, metallicity, and age and can be altered by binarity. To understand the importance of these parameters in main-sequence stars, we...



