The Impact of Rotation on the Evolution of Low–Mass Stars
نویسندگان
چکیده
High precision photometry and spectroscopy of low–mass stars reveal a variety of properties standard stellar evolution cannot predict. Rotation, an essential ingredient of stellar evolution, is a step towards resolving the discrepancy between model predictions and observations. The first rotating stellar model, continuously tracing a low–mass star from the pre–main sequence onto the horizontal branch, is presented. The predicted luminosity functions of globular clusters and surface rotation velocities on the horizontal branch are discussed.
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