EVOLUTION OF STELLAR MODELS WITH HIGH METAL CONTENT

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Date

1971

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UNAM, Boletín de Observatorios Tonatzintla y Tacubaya, México.
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Abstract

Evolutionary sequences for stellar configurations between 1 and 1.45 /b M//sub o/ with chemical abundances varying from /b Z/=0.023 to 0.10 and from /b X/=0.60 to 0.68 were computed using the Berkeley Stellar Evolution program. The effect of high metal ab

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Keywords

EVOLUTION, STELLAR, MODELS, HIGH, METAL CONTENT

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https://ahcm.cinvestav.mx/handle/ahcm/23140

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