THE EFFECT OF CHEMICAL ABUNDANCE OSCILLATIONS ON THE PULSATIONAL PROPERTIES OF A 5 M-CIRCLE-DOT HYDROGEN-HELIUM STAR
ASTROPHYSICS AND SPACE SCIENCE, vol.192, no.2, pp.275-289, 1992 (SCI-Expanded, Scopus)
- Publication Type: Article / Article
- Volume: 192 Issue: 2
- Publication Date: 1992
- Doi Number: 10.1007/bf00684485
- Journal Name: ASTROPHYSICS AND SPACE SCIENCE
- Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
- Page Numbers: pp.275-289
- Middle East Technical University Affiliated: No
Abstract
A model of a first generation intermediate star of 5 M., with Z = 0 has been considered. The model is at an advanced stage of its evolution and has a double shell burning. It burns helium in the inner shell, and hydrogen, via CNO cycle, in the outer shell.