arXiv · 1210.3505
Determination of the stars fundamental parameters using seismic scaling relations
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.
Explore related subjects
Keep this discovery
K. Belkacem. 2012-10-12. Determination of the stars fundamental parameters using seismic scaling relations. https://arxiv.org/abs/1210.3505
Cite the original work for its findings. Save a collection to share your selection of sources.