Main sequence for rotating stars of intermediate mass

DOI10.1007/BF00644173zbMath0615.70005OpenAlexW2079718893MaRDI QIDQ1820605

N. Özkara, D. Eryurt-Ezer, H. Kirbiyik

Publication date: 1986

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00644173

zbMATH Keywords

rotational instabilitycritical rotationevolutionary behaviourfast rotation modelHertzsprung- Russell diagramintermediate massPopulation I starsslow rotation modelthreshold of stabilityzero-age main sequence

Mathematics Subject Classification ID

Computational methods for problems pertaining to mechanics of particles and systems (70-08) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05)

Cites Work

• A New Method of Automatic Computation of Stellar Evolution.

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