NASA NTRS · 19690049587
A criterion for nuclear-energized pulsational instability.
Abstract
Nuclear energized pulsational instability of stars based on linear quasi-adiabatic theory, including models with hydrogen burning shells
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Simon, N. R., Stothers, R.. 1969-04-01. A criterion for nuclear-energized pulsational instability.. https://ntrs.nasa.gov/citations/19690049587
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