Stellar model fits and inversions
arXiv:1211.2697 · doi:10.1002/asna.201211836
Abstract
The recent asteroseismic data from the CoRoT and Kepler missions have provided an entirely new basis for investigating stellar properties. This has led to a rapid development in techniques for analysing such data, although it is probably fair to say that we are still far from having the tools required for the full use of the potential of the observations. Here I provide a brief overview of some of the issues related to the interpretation of asteroseismic data.
Proc. ESF Conference : "The Modern Era of Helio- and Asteroseismology", Obergurgl, 20 - 25 May, 2012. To appear in Astron. Nach. Guest editor: Markus Roth
References in corpus (19)
- Spin down of the core rotation in red giants
- ADIPLS -- the Aarhus adiabatic oscillation package
- Seismic evidence for a rapidly rotating core in a lower-giant-branch star observed with Kepler
- Correcting stellar oscillation frequencies for near-surface effects
- ASTEC -- the Aarhus STellar Evolution Code
- Fundamental Properties of Stars using Asteroseismology from Kepler & CoRoT and Interferometry from the CHARA Array
- Asteroseismology of the solar analogs 16 Cyg A & B from Kepler observations
- Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission
- Verifying asteroseismically determined parameters of Kepler stars using hipparcos parallaxes: self-consistent stellar properties and distances
- Oscillation mode frequencies of 61 main sequence and subgiant stars observed by Kepler
- A precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764
- An asteroseismic signature of helium ionization
- Oscillating K giants with the WIRE satellite: determination of their asteroseismic masses
- A Stellar Model-fitting Pipeline for Asteroseismic Data from the Kepler Mission
- Asteroseismic Signatures of Small Convective Cores
- A Bayesian approach to the modelling of alpha Cen A
- AMP: A Science-driven Web-based Application for the TeraGrid
- Porto Oscillation Code (POSC)
- Asteroseismology of red giants
Cited by in corpus (19)
- Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology
- Testing the asteroseismic scaling relations for Red Giants with Eclipsing Binaries Observed by Kepler
- Giant star seismology
- Kepler-91b: a planet at the end of its life. Planet and giant host star properties via light-curve variations
- First Results From The Hertzsprung Song Telescope: Asteroseismology Of The G5 Subgiant Star {\Mu}Her
- Interaction Between Convection and Pulsation
- Asteroseismic modeling of 16 Cyg A & B using the complete Kepler data set
- Uncertainties in grid-based estimates of stellar mass and radius. SCEPtER: Stellar CharactEristics Pisa Estimation gRid
- KIC 9246715: The Double Red Giant Eclipsing Binary With Odd Oscillations
- SpaceInn hare-and-hounds exercise: Estimation of stellar properties using space-based asteroseismic data
- A prescription for the asteroseismic surface correction
- Asteroseismic g-mode period spacings in strongly magnetic rotating stars
- Detection of Solar-Like Oscillations, Observational Constraints, and Stellar Models for Cyg, the Brightest Star Observed by the {\it Kepler} Mission
- CoRoT and Kepler results: Solar-like oscillators
- Damping rates and frequency corrections of Kepler LEGACY stars
- Coupling between turbulence and solar-like oscillations: a combined Lagrangian PDF/SPH approach. I -- The stochastic wave equation
- Coupling between turbulence and solar-like oscillations: A combined Lagrangian PDF/SPH approach. II - Mode driving, damping and modal surface effect
- Inverse analysis of asteroseismic data: a review
- Calibrating damping rates with LEGACY linewidths