Physics
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980cpsp.book..363s&link_type=abstract
In NASA. Goddard Space Flight Center Current Probl. in Stellar Pulsation Instabilities p 363-380 (SEE N80-25229 15-90)
Physics
1
Cepheus Constellation, Stellar Evolution, Variable Stars, Angular Velocity, Kelvin-Helmholtz Instability, Stellar Mass
Scientific paper
The evolutionary aspects of massive population 1 stars were investigated. Semiconvection was treated in two different ways, and included mass loss both in the early as well as later spectra stages. The effect of rotation was taken into account and the time evolution of angular momentum of these models was studied. The effect of differential rotation due to the faster rotating interiors and slowed down surface layers are briefly described.
Ranga Sreenivasan S.
Wilson J. F. W.
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