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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

A. V. Sweigart ,
L. Greggio  and
A. Renzini
A. V. Sweigart
Affiliation:
NASA Goddard Space Flight Center
L. Greggio
Affiliation:
University of Bologna
A. Renzini
Affiliation:
University of Bologna

Abstract

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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.

Type
Chapter VII. Poster Papers on Harlow Shapley and Globular Clusters in the Milky Way
Information
Symposium - International Astronomical Union , Volume 126: The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies , 1988 , pp. 483 - 484
Copyright
Copyright © Kluwer 1988 

References

REFERENCE

Sweigart, A. V., and Gross, P. G. 1978 Astrophys. J. Suppl. 36, 405.Google Scholar