How accurate are stellar ages based on stellar models? II. The impact of asteroseismology
arXiv:1410.5337 · doi:10.1051/eas/1465005
Abstract
Accurate and precise stellar ages are best determined for stars which are strongly observationally constrained, that is which are intrinsically oscillating. We review here the seismic diagnostics which are sensitive to stellar ages and provide some illustrating examples of seismically age-dated stars.
arXiv comment49 pages, 20 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 (68)
- The chemical composition of the Sun
- Kepler Mission Design, Realized Photometric Performance, and Early Science
- GAIA: Composition, Formation and Evolution of the Galaxy
- Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars
- Asteroseismology of Solar-Type and Red-Giant Stars
- Spin down of the core rotation in red giants
- Seismic evidence for a rapidly rotating core in a lower-giant-branch star observed with Kepler
- Asteroseismic fundamental properties of solar-type stars observed by the NASA Kepler Mission
- Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants
- Correcting stellar oscillation frequencies for near-surface effects
- Seismic diagnostics for transport of angular momentum in stars 1. Rotational splittings from the PMS to the RGB
- Probing the core structure and evolution of red giants using gravity-dominated mixed modes observed with Kepler
- Probing the properties of convective cores through g modes: high-order g modes in SPB and gamma Doradus stars
- Solar-like oscillations in low-luminosity red giants: first results from Kepler
- Red-giant seismic properties analyzed with CoRoT
- The underlying physical meaning of the relation
- Theoretical amplitudes and lifetimes of non-radial solar-like oscillations in red giants
- Galactic archaeology: mapping and dating stellar populations with asteroseismology of red-giant stars
- Angular momentum transport in stellar interiors constrained by rotational splittings of mixed modes in red giants
- A uniform asteroseismic analysis of 22 solar-type stars observed by Kepler
- Asteroseismology of the solar analogs 16 Cyg A & B from Kepler observations
- Mixed modes in red-giant stars observed with CoRoT
- Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission
- Detection of Solar-like Oscillations in the G7 Giant Star xi Hya
- Characteristics of solar-like oscillations in red giants observed in the CoRoT exoplanet field
- Constraining fundamental stellar parameters using seismology. Application to Alpha Centauri AB
- Asteroseismology for "à la carte" stellar age-dating and weighing: Age and mass of the CoRoT exoplanet host HD 52265
- A precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764
- Asymptotic and measured large frequency separations
- How much do helioseismological inferences depend upon the assumed reference model?
- Oscillations of alpha UMa and other red giants
- Stellar ages and convective cores in field main-sequence stars: first asteroseismic application to two Kepler targets
- Probing populations of red giants in the galactic disk with CoRoT
- A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology
- Seismic diagnostics for transport of angular momentum in stars 2. Interpreting observed rotational splittings of slowly-rotating red giant stars
- Constraints on the structure of the core of subgiants via mixed modes: the case of HD49385
- Testing convective-core overshooting using period spacings of dipole modes in red giants
- A Stellar Model-fitting Pipeline for Asteroseismic Data from the Kepler Mission
- Characterisation of red-giant stars in the public Kepler data
- An asteroseismic membership study of the red giants in three open clusters observed by Kepler: NGC6791, NGC6819, and NGC6811
- Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265
- Kepler-68: Three Planets, One With a Density Between That of Earth and Ice Giants
- Seismic and spectroscopic characterization of the solar-like pulsating CoRoT target HD 49385
- Seismic diagnostics of red giants: first comparison with stellar models
- A large sample of calibration stars for Gaia: log g from Kepler and CoRoT
- Automatic Determination of Stellar Parameters via Asteroseismology of Stochastically Oscillating Stars: Comparison with Direct Measurements
- Asteroseismology of the Transiting Exoplanet Host HD 17156 with HST FGS
- Solar-like oscillations in KIC11395018 and KIC11234888 from 8 months of Kepler data
- Detection of solar-like oscillations from Kepler photometry of the open cluster NGC 6819
- A Bayesian approach to the modelling of alpha Cen A
- Asteroseismic modelling of the solar-type subgiant star Hydri
- Asteroseismic diagrams for solar-type stars
- Precise Estimates of the Physical Parameters for the Exoplanet System HD-17156 Enabled by HST FGS Transit and Asteroseismic Observations
- Toward a New Kind of Asteroseismic Grid Fitting
- Atmospheric parameters and chemical properties of red giants in the CoRoT asteroseismology fields
- New insights on the interior of solar-like pulsators thanks to CoRoT: the case of HD 49385
- Assessing the accuracy of the gravity determination in late-type stars with solar-like pulsators
- Masses of subgiant stars from asteroseismology using the coupling strengths of mixed modes
- Asteroseismology of red giants as a tool for studying stellar populations: first steps
- Precise Modeling of the Exoplanet Host Star and CoRoT Main Target HD 52265
- Seismic signature of envelope penetrative convection: the CoRoT star HD 52265
- Characterizing two solar-type Kepler subgiants with asteroseismology: KIC10920273 and KIC11395018
- 12 Bootis: a test bed for extra-mixing processes in stars
- On Limiting the Thickness of the Solar Tachocline
- Abundance study of the two solar-analogue CoRoT targets HD 42618 and HD 43587 from HARPS spectroscopy
- Seismic analysis of HD43587Aa, a solar-like oscillator in a multiple system
- Asteroseismology of red giant stars: the potential of dipole modes
- Impact of asteroseismology on improving stellar ages determination
Cited by in corpus (25)
- Probing the interior physics of stars through asteroseismology
- Asteroseismology of solar-type stars
- Population synthesis to constrain Galactic and Stellar Physics- I- Determining age and mass of thin-disc red-giant stars
- Asteroseismology of red giants: from analysing light curves to estimating ages
- Using seismic inversions to obtain an internal mixing processes indicator for main-sequence solar-like stars
- Cluster Ages to Reconstruct the Milky Way Assembly (CARMA) I. The final word on the origin of NGC6388 and NGC6441
- The PLATO Solar-like Light-curve Simulator: A tool to generate realistic stellar light-curves with instrumental effects representative of the PLATO mission
- The evolution of the Milky Way's thin disc radial metallicity gradient with K2 asteroseismic ages
- Deciphering the evolution of the Milky Way discs: Gaia APOGEE Kepler giant stars and the Besançon Galaxy Model
- Magnetic signatures on mixed-mode frequencies. II. Period spacings as a probe of the internal magnetism of red giants
- Differential Modelling Systematics across the HR Diagram from Asteroseismic Surface Corrections
- Influence of metallicity on the near-surface effect on oscillation frequencies
- On attempting to automate the identification of mixed dipole modes for subgiant stars
- On the characterization of GJ 504: a magnetically active planet-host star observed by the Transiting Exoplanet Survey Satellite (TESS)
- A binary with a ~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821
- Asteroseismic age estimates of RGB stars in open clusters. A statistical investigation of different estimation methods
- Clusters: age scales for stellar physics
- Relevance of the small frequency separation for asteroseismic stellar age, mass, and radius. A statistical investigation for main-sequence low-mass stars
- The age of the Methuselah star in light of stellar evolution models with tailored abundances
- A catalogue of asteroseismically calibrated ages for APOGEE DR17. The predictions of a CatBoost machine learning model based on the [Mg/Ce] chemical clock and other stellar parameters
- New stellar age estimates using SPInS based on Gaia DR3 photometry and LAMOST DR8 abundances
- Properties of observable mixed inertial and gravito-inertial modes in γ Doradus stars
- The impact of the transport of chemicals and electronic screening on helioseismic and neutrino observations in solar models
- Stellar age determination using deep neural networks: Isochrone ages for 1.3 million stars, based on BaSTI, MIST, PARSEC, Dartmouth and SYCLIST evolutionary grids
- The SAGA so far: reading the history of the Galaxy with asteroseismology