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Instability of radial oscillations of Wolf-Rayet star models
Date
1987
Author
Kırbıyık, Halil
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By taking some evolutionary models of an initially 60M ⊙-star, their radial vibrational stabilities have been investigated. These models, evolving with mass loss, are in the advanced stages of their evolution, and burn He in their cores. Calculations have been performed for the first and second harmonics as well as for the fundamental mode; and some of these models were found to be vibrationally unstable in the fundamental mode.
Subject Keywords
Space and Planetary Science
,
Astronomy and Astrophysics
URI
https://hdl.handle.net/11511/51987
Journal
Astrophysics and Space Science
DOI
https://doi.org/10.1007/bf00642123
Collections
Department of Physics, Article
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H. Kırbıyık, “Instability of radial oscillations of Wolf-Rayet star models,”
Astrophysics and Space Science
, pp. 321–330, 1987, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/51987.