A seismic scaling relation for stellar age
arXiv:1903.03110 · doi:10.1093/mnras/stz714
Abstract
A simple solar scaling relation for estimating the ages of main-sequence stars from asteroseismic and spectroscopic data is developed. New seismic scaling relations for estimating mass and radius are presented as well, including a purely seismic radius scaling relation (i.e., no dependence on temperature). The relations show substantial improvement over the classical scaling relations and perform similarly well to grid-based modeling.
10 pages, including source code. Accepted for publication in MNRAS
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Cited by in corpus (5)
- A seismic scaling relation for stellar age II: The red giant branch
- Testing stellar evolution with asteroseismic inversions of a main sequence star harboring a small convective core
- Asteroseismic Investigation of 20 Planet and Planet-Candidate Host Stars
- TATOO: a tidal-chronology standalone tool to estimate the age of massive close-in planetary systems
- Scaling relations for solar-like oscillations: a review