Department of Physics and Astronomy: Publications and Other Research
Document Type
Article
Date of this Version
1970
Abstract
Simple analytical relations are derived - similar to the homology relations for homogeneous stam - which describe the behaviour of shell source burning models with highly condensed cores. Many features which are known from evolutionary calculations (and partly &om observations) of such stars can be understood as coming essentially from the increase of the mass M6 of the core.
Comments
Published in Astronomy & Astrophy. 6, 426-440, 1970. Used by permission.