Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 486, Issue 4, Pages 4612-4621Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz714
Keywords
asteroseismology; stars: evolution; stars: fundamental parameters; stars: solar-type
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Funding
- Danish National Research Foundation [DNRF106]
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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 modelling.
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