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The Development of a Red-Giant Branch in Low to Intermediate Mass Stars
Published online by Cambridge University Press: 19 July 2016
Abstract
A new grid of evolutionary sequences has been computed for the main sequence and first red-giant branch (RGB) phases of low to intermediate mass stars. From these sequences we have obtained new intermediate age isochrones.
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- Chapter VII. Poster Papers on Harlow Shapley and Globular Clusters in the Milky Way
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- Copyright © Kluwer 1988