Non-radial oscillations and vibrational stability of massive stars initially composed of pure hydrogen
Date
1966
Authors
Wan Fook Sun
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Abstract
The study of vibrational stability of nassive stars undergoing
radial oscillations has been investigated thoroughly by Schwarzschild
and Harm [1], A. Boury [2] and P. Ledoux [3]. However, until
recentl~ very little work has been done on the stability of stars
undergoing non-radial oscillations. R.L. Simon [4] has studied the
vibrational stability of the standard model undergoing non-radial
oscillations but the difficulty in solving the basic equations governing
non-radial oscillations has hampered the study of the stability of
massive stars.
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Thesis (PhD)
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