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Observational tests for overshoot and opacity enhancement based on massive stars
Published online by Cambridge University Press: 04 August 2017
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It is shown that a moderate increase in the opacity due to heavy elements in models of massive stars, incorporating convective overshoot and mass loss by stellar wind, can remove the well known discrepancy between theoretical expectation and observed frequencies of luminous stars in the HR diagram. These models in fact extend their main sequence band far beyond the classical limit.
- Type
- II. EVOLUTION OF MASSIVE STARS EVOLUTION AND MODELS
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- Copyright © Reidel 1984
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