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pro vyhledávání: '"Bu, Yutian"'
Many young clusters possess extended main sequences, a phenomenon commonly ascribed to stellar rotation. However, the mechanism behind their very wide stellar rotation distributions remains unclear. A proposed explanation is that magnetic star-disk i
Externí odkaz:
http://arxiv.org/abs/2412.00520
Research has shown that many young and intermediate-age clusters (younger than $\sim$2 Gyr) have extended main sequences and main-sequence turnoffs (eMSTOs), which cannot be adequately described by a single isochrone. The reason for the extended main
Externí odkaz:
http://arxiv.org/abs/2404.12331