Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980azh....57.1273f&link_type=abstract
(Astronomicheskii Zhurnal, vol. 57, Nov.-Dec. 1980, p. 1273-1276.) Soviet Astronomy, vol. 24, Nov.-Dec. 1980, p. 733-735. Trans
Astronomy and Astrophysics
Astronomy
Electron Gas, Main Sequence Stars, Stellar Gravitation, Stellar Magnetic Fields, Stellar Mass, Stellar Rotation, Angular Momentum, Chemical Composition, Equations Of State, Hertzsprung-Russell Diagram, Nonuniform Magnetic Fields, Poloidal Flux, Stellar Evolution
Scientific paper
The present study examines the influence of rigid-body and differential rotation and of a fine-scale chaotic magnetic field and a poloidal magnetic field on the minimum mass of a main sequence star. Calculations are performed with allowance for two main effects in the equation of state: ionization and dissociation by pressure and the partial degeneracy of the electron gas. It is shown that rotation and a magnetic field with an energy equal to 10-20% of the star's gravitational energy increase the minimum mass of a main sequence star by 1.5-2 times.
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