No CrossRef data available.
Article contents
Modeling the global oscillations of Epsilon Eridani
Published online by Cambridge University Press: 03 August 2017
Abstract
We have reviewed the observational data for ∊ Eri to derive our best estimates of luminosity, radius, temperature, composition, and age, as well as the uncertainties associated with each of these. These quantities are then used in stellar structure models to try to reproduce the global oscillation frequencies observed by Noyes et al. We find that we can reproduce the observed frequencies and splittings at least as well as the computations of Guenther and Demarque, yet for significantly different stellar parameters, most notably the age.
- Type
- Chapter 4: Asteroseismology: Results and Prospects
- Information
- Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 281 - 284
- Copyright
- Copyright © Reidel 1988