Semiconvection in halo stars and primordial helium abundance

Semiconvection in halo stars and primordial helium abundance

Convective overshooting and semiconvection in core-helium burning stars are studied with emphasis on laboratory experiments and terrestrial observations. A necessary condition for the onset of semiconvection is derived, and the Schwarzschild neutrality criterion for the semiconvective zone is justif...

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Bibliographic Details
Main Author: Tarbell, Theodore Dean
Format: Others
Published: 1976
Online Access:https://thesis.library.caltech.edu/4289/1/Tarbell_td_1976.pdf
Tarbell, Theodore Dean (1976) Semiconvection in halo stars and primordial helium abundance. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/J7AW-9943. https://resolver.caltech.edu/CaltechETD:etd-10282008-143946 <https://resolver.caltech.edu/CaltechETD:etd-10282008-143946>

Internet

https://thesis.library.caltech.edu/4289/1/Tarbell_td_1976.pdf
Tarbell, Theodore Dean (1976) Semiconvection in halo stars and primordial helium abundance. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/J7AW-9943. https://resolver.caltech.edu/CaltechETD:etd-10282008-143946 <https://resolver.caltech.edu/CaltechETD:etd-10282008-143946>

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