Asteroseismic age determination for dwarfs and giants
V. Silva Aguirre, A. M. Serenelli
TL;DR
This paper reviews how asteroseismology helps determine stellar ages and properties, enhancing our understanding of the Milky Way's history with current results and future improvements.
Contribution
It summarizes the observables, precision levels, current age estimates, and future prospects of asteroseismic stellar property determination for Galactic archaeology.
Findings
Asteroseismology provides precise stellar properties.
Current age estimates for dwarfs and giants are improving.
Future data will enhance Galactic evolutionary models.
Abstract
Asteroseismology can make a substantial contribution to our understanding of the formation history and evolution of our Galaxy by providing precisely determined stellar properties for thousands of stars in different regions of the Milky Way. We present here the different sets of observables used in determining asteroseismic stellar properties, the typical level of precision obtained, the current status of results for ages of dwarfs and giants and the improvements than can be expected in the near future in the context of Galactic archaeology.
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