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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
Metadata
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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
Citation Formats
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MLA
BibTeX
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.
