Low-mass pre-main-sequence stars in Taurus-Auriga
收藏B2FIND2026-04-04 收录
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https://b2find.eudat.eu/dataset/01dc1664-c798-57aa-ae0e-6d92594cc931
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The projected stellar rotational velocity (vsini) is critical for our understanding of processes related to the evolution of angular momentum in pre-main-sequence stars. We...
