THE EFFECT OF CHEMICAL ABUNDANCE OSCILLATIONS ON THE PULSATIONAL PROPERTIES OF A 5 M-CIRCLE-DOT HYDROGEN-HELIUM STAR

Date

1992-06-01

Author

UYANIKER, B
KIRBIYIK, H

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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.

Subject Keywords

Space and Planetary Science, Astronomy and Astrophysics

URI

https://hdl.handle.net/11511/64519

Journal

ASTROPHYSICS AND SPACE SCIENCE

DOI

https://doi.org/10.1007/bf00684485

Collections

Department of Physics, Article

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Citation Formats

B. UYANIKER and H. KIRBIYIK, “THE EFFECT OF CHEMICAL ABUNDANCE OSCILLATIONS ON THE PULSATIONAL PROPERTIES OF A 5 M-CIRCLE-DOT HYDROGEN-HELIUM STAR,” ASTROPHYSICS AND SPACE SCIENCE, pp. 275–289, 1992, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/64519.