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Evidence for a main sequence widening for massive stars
Published online by Cambridge University Press: 04 August 2017
Extract
Theoretical isochrones, in the interval 3 to 25 106 y., have been obtained from the grid of stellar models with mass loss computed by Maeder (1980, 1981). They cover the main sequence evolution, the red supergiant region and the first blue loop. These isochrones have been compared to composite colour magnitude diagrams of young open clusters drawn by Mermilliod (1981).
- Type
- II. EVOLUTION OF MASSIVE STARS EVOLUTION AND MODELS
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- Copyright © Reidel 1984
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