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Theoretical horizontal-branch evolutionThe general features of the theoretical evolution of canonical horizontal-branch (HB) stars are briefly reviewed with specific emphasis on the track morphology in the HR diagram and the determination of the globular cluster helium abundance. The observational evidence for the occurrence of semiconvection is discussed together with some remaining theoretical uncertainty.
Document ID
19890030160
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Sweigart, Allen V.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1987
Subject Category
Astrophysics
Meeting Information
Meeting: Conference on Faint Blue Stars
Location: Tucson, AZ
Country: United States
Start Date: June 1, 1987
End Date: June 5, 1987
Sponsors: IAU, NSF
Accession Number
89A17531
Distribution Limits
Public
Copyright
Other

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