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A criterion for nuclear-energized pulsational instability.Nuclear energized pulsational instability of stars based on linear quasi-adiabatic theory, including models with hydrogen burning shells
Document ID
19690049587
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Simon, N. R.
Stothers, R.
Date Acquired
August 5, 2013
Publication Date
April 1, 1969
Subject Category
Space Sciences
Accession Number
69A27576
Distribution Limits
Public
Copyright
Other

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