# Determination of the stars fundamental parameters using seismic scaling relations

Source: [Determination of the stars fundamental parameters using seismic scaling relations](<https://www.sota2.com/research/paper/68fa2ba91e209131ce848abe>)

Collection index: [llms.txt](<https://www.sota2.com/research/llms.txt>)

Data updated: 2025-10-24T14:19:48.651Z

Authors: K. Belkacem

Published: 2012-10-12T13:11:28.000Z

## Abstract

Seismology of stars that exhibit solar-like oscillations develops a growing interest with the wealth of observational results obtained with the CoRoT and Kepler space-borne missions. In this framework, relations between asteroseismic quantities and stellar parameters provide a unique opportunity to derive model-independent determinations of stellar parameters (e.g., masses and radii) for a large sample of stars. I review those scaling relations with particular emphasis on the underlying physical processes governing those relations, as well as their uncertainties.

## Recorded benchmark results

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## Original sources and implementation

[Original paper](<https://arxiv.org/abs/1210.3505>)

[PDF](<https://arxiv.org/pdf/1210.3505.pdf>)