Granulation model for 508 KIC stars
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/2e0e642d-caf3-5332-8c14-31c669c396c0
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A large fraction of cool, low-mass stars exhibit brightness fluctuations that arise from a combination of convective granulation, acoustic oscillations, magnetic activity, and...



