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)