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Effects of New Opacity on the Post-AGB Evolution
Published online by Cambridge University Press: 07 August 2017
Abstract
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Using the OPAL opacity, we have calculated the post-AGB evolutions of low mass stars. It is newly found that optically thick wind occurs for Mcore > 0.55M⊙ and the evolutionary time scale is drastically shortened.
- Type
- IV. Planetary Nebulae Connection: Evolution from the AGB
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- Copyright
- Copyright © Kluwer 1993
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