The ATON 3.1 stellar evolutionary code

@article{Ventura2008TheA3,
  title={The ATON 3.1 stellar evolutionary code},
  author={P. Ventura and F. D'antona and I. Mazzitelli},
  journal={Astrophysics and Space Science},
  year={2008},
  volume={316},
  pages={93-98}
}
  • P. Ventura, F. D'antona, I. Mazzitelli
  • Published 2008
  • Physics
  • Astrophysics and Space Science
    • Abstract We describe the main features of the evolutionary code ATON 3.1 and its latest version, particularly deviced to be apt for follow up asteroseismology applications. An older version of the code including rotational evolution is also shortly described.  
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    References

    SHOWING 1-10 OF 33 REFERENCES
    THE EVOLUTION OF ROTATING STARS
    • 545
    • PDF
    Studies in Stellar Evolution. III. The Calculation of Model Envelopes.
    • 169
    The evolution of rotating stars. I - Method and exploratory calculations for a 7-solar-mass star
    • 170
    Non-gray rotating stellar models and the evolutionary history of the Orion Nebular Cluster
    • 17
    • PDF
    Updated and Expanded OPAL Equation-of-State Tables: Implications for Helioseismology
    • 522
    • PDF
    Updated Electron-Conduction Opacities: The Impact on Low-Mass Stellar Models
    • 216
    • PDF
    Structure and evolution of low-mass Population II stars
    • 3
    • PDF
    Lithium and mass loss in massive AGB stars in the Large Magellanic Cloud
    • 2
    • PDF
    85 Peg A: what age for a low-metallicity solar-like star?
    • 14
    • PDF
    A Simple Method for the Solution of the Stellar Structure Equations Including Rotation and Tidal Forces
    • 110