Bayesian asteroseismology of 23 solar-like Kepler targets
- Autor(en)
- M. Gruberbauer, D. B. Guenther, K. MacLeod, T. Kallinger
- Abstrakt
We study 23 previously published Kepler targets to perform a consistent
grid-based Bayesian asteroseismic analysis and compare our results to
those obtained via the Asteroseismic Modelling Portal. We find
differences in the derived stellar parameters of many targets and their
uncertainties. While some of these differences can be attributed to
systematic effects between stellar evolutionary models, we show that the
different methodologies deliver incompatible uncertainties for some
parameters. Using non-adiabatic models and our capability to measure
surface effects, we also investigate the dependency of these surface
effects on the stellar parameters. Our results suggest a dependence of
the magnitude of the surface effect on the mixing length parameter which
also, but only minimally, affects the determination of stellar
parameters. While some stars in our sample show no surface effect at
all, the most significant surface effects are found for stars that are
close to the Sun's position in the Hertzsprung-Russell diagram.
- Organisation(en)
- Institut für Astrophysik
- Externe Organisation(en)
- Saint Mary's University
- Journal
- Monthly Notices of the Royal Astronomical Society
- Band
- 435
- Seiten
- 242-254
- Anzahl der Seiten
- 13
- ISSN
- 0035-8711
- DOI
- https://doi.org/10.1093/mnras/stt1289
- Publikationsdatum
- 10-2013
- Peer-reviewed
- Ja
- ÖFOS 2012
- 103004 Astrophysik, 103003 Astronomie
- Schlagwörter
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/2e24a58e-9df6-4202-9c83-e7f3276964ef