Review paper
The Evolution of Low Mass Stars
Volume: 151, Issue: 3, Pages: 351 - 364
Published: Feb 1, 1971
Abstract
This paper presents a method of computing the evolution of low mass stars from the main sequence to the helium flash. Many such computations are handicapped by the fact that the hydrogen burning shell source becomes very thin at a relatively early stage of evolution, and this means that either a very short time step is needed on the red giant branch, or else that some special method must be introduced. The present method has neither handicap:...
Paper Details
Title
The Evolution of Low Mass Stars
Published Date
Feb 1, 1971
Volume
151
Issue
3
Pages
351 - 364
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