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The contraction phase of solar evolution.Gravitational contraction of stars of one solar mass examined, using Henyey method for calculating stellar evolutionary tracks
Document ID
19660057501
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cameron, A. G. W.
Ezer, D.
Date Acquired
August 3, 2013
Publication Date
January 1, 1966
Subject Category
Space Sciences
Accession Number
66A36791
Distribution Limits
Public
Copyright
Other
Keywords
GRAVITATIONAL COLLAPSE
DYNAMIC STABILITY
STELLAR EVOLUTION

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