Show/Hide Menu
Hide/Show Apps
anonymousUser
Logout
Türkçe
Türkçe
Search
Search
Login
Login
OpenMETU
OpenMETU
About
About
Açık Bilim Politikası
Açık Bilim Politikası
Frequently Asked Questions
Frequently Asked Questions
Browse
Browse
By Issue Date
By Issue Date
Authors
Authors
Titles
Titles
Subjects
Subjects
Communities & Collections
Communities & Collections
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
Show full item record
This work is licensed under a
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
.
Item Usage Stats
2
views
0
downloads
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
