How accurate are stellar ages based on stellar models ? I. The impact of stellar models uncertainties
arXiv:1410.5336 · doi:10.1051/eas/1465004
Abstract
Among the various methods used to age-date stars, methods based on stellar model predictions are widely used, for nearly all kind of stars in large ranges of masses, chemical compositions and evolutionary stages. The precision and accuracy on the age determination depend on both the precision and number of observational constraints, and on our ability to correctly describe the stellar interior and evolution. The imperfect input physics of stellar models as well as the uncertainties on the initial chemical composition of stars are responsible for uncertainties in the age determination. We present an overview of the calculation of stellar models and discuss the impact on age of their numerous inputs.
83 pages, 46 figures, contribution to the proceedings of the 13rd Evry Schatzman School on Stellar Astrophysics, "The Ages of Stars", Roscoff 2013, EAS Publications Series, eds. Y. Lebreton, D. Valls-Gabaud, C. Charbonnel
References in corpus (22)
- Modules for Experiments in Stellar Astrophysics (MESA)
- Updated Electron-Conduction Opacities: The Impact on Low-Mass Stellar Models
- Basic physical parameters of a selected sample of evolved stars
- Helioseismology and Solar Abundances
- A Bitter Pill: The Primordial Lithium Problem Worsens
- A probable stellar solution to the cosmological lithium discrepancy
- CESAM: a free code for stellar evolution calculations
- Rotational mixing in low-mass stars II. Self-consistent models of Pop II RGB stars
- The Liege Oscillation Code
- LUNA: Nuclear Astrophysics Deep Underground
- Precision study of ground state capture in the 14N(p,gamma)15O reaction
- Magnetic confinement of the solar tachocline: II. Coupling to a convection zone
- First full evolutionary computation of the He-flash induced mixing in Population II stars
- On the proper use of the Schwarzschild and Ledoux criteria in stellar evolution computations
- A synoptic comparison of the MHD and the OPAL equations of state
- CoRoT/ESTA-TASK 1 and TASK 3 comparison of the internal structure and seismic properties of representative stellar models: Comparisons between the ASTEC, CESAM, CLES, GARSTEC and STAROX codes
- Transport processes in stars: diffusion, rotation, magnetic fields and internal waves
- The CoRoT Evolution and Seismic Tools Activity: Goals and Tasks
- The new Toulouse-Geneva Stellar Evolution Code including radiative accelerations of heavy elements
- Dynamic screening correction for solar p-p reaction rates
- Thorough analysis of input physics in CESAM and CLES codes
- Radiation-hydrodynamics simulations of surface convection in low-mass stars: connections to stellar structure and asteroseismology
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- The age of the Methuselah star in light of stellar evolution models with tailored abundances
- New stellar age estimates using SPInS based on Gaia DR3 photometry and LAMOST DR8 abundances
- The GALAH survey: Multiple stars and our Galaxy. I. A comprehensive method for deriving properties of FGK binary stars
- Uncertainties in asteroseismic grid-based estimates of the ages of halo stars
- Asteroseismically Inferred Ages of 132,000 Red Giants with TESS
- The oldest Milky Way stars: New constraints on the age of the Universe and the Hubble constant
- Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn
- The impact of the transport of chemicals and electronic screening on helioseismic and neutrino observations in solar models
- Asteroseismic modelling of main-sequence solar-like stars and Kepler exoplanet host stars with the FICO procedure I. Catalogue of fundamental stellar properties
- Stellar age determination using deep neural networks: Isochrone ages for 1.3 million stars, based on BaSTI, MIST, PARSEC, Dartmouth and SYCLIST evolutionary grids