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The evolution of population II stars.Evolutionary paths of several double energy-source models compared with horizontal branch in metal- weak Population II clusters to obtain stellar structure and mass for best fit
Document ID
19660054855
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/148697
Authors
Faulkner, J.
Iben, I., Jr.
Date Acquired
August 3, 2013
Publication Date
June 1, 1966
Publication Information
Publication: ASTROPHYSICAL JOURNAL
Subject Category
Space Sciences
Accession Number
66A34145
Funding Number(s)
CONTRACT_GRANT: NSF GP-5391
CONTRACT_GRANT: NONR-220/47/
CONTRACT_GRANT: NSG-496
Distribution Limits
Public
Copyright
Other
Keywords
STELLAR STRUCTURE
STELLAR EVOLUTION

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