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

1992-06-01
UYANIKER, B
KIRBIYIK, H
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.

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, vol. 192, no. 2, pp. 275–289, 1992, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/64519.