On the semiconvective zone in the core-helium-burning stars

Hideyuki Saio

doi:10.1007/BF00642717

On the semiconvective zone in the core-helium-burning stars

Hideyuki Saio

Research output: Contribution to journal › Article › peer-review

Abstract

The validity of current ideas to set up the semiconvective zone of the stellar models in corehelium-burning phase has been considered mainly from the view point of times-cales related to the mechanism. The time-scale of outward motion of convective shell has been estimated as being longer than that of evolution. From this point of view, it might be said that the models constructed with semiconvective zone are not appropriate for the core-helium-burning stars.

Original language	English
Pages (from-to)	41-49
Number of pages	9
Journal	Astrophysics and Space Science
Volume	29
Issue number	1
DOIs	https://doi.org/10.1007/BF00642717
Publication status	Published - 1974 Jul
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1007/BF00642717

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title = "On the semiconvective zone in the core-helium-burning stars",

abstract = "The validity of current ideas to set up the semiconvective zone of the stellar models in corehelium-burning phase has been considered mainly from the view point of times-cales related to the mechanism. The time-scale of outward motion of convective shell has been estimated as being longer than that of evolution. From this point of view, it might be said that the models constructed with semiconvective zone are not appropriate for the core-helium-burning stars.",

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On the semiconvective zone in the core-helium-burning stars

Abstract

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