Modeling epsilon Eridani and its oscillations

@inproceedings{Soderblom1989ModelingEE,
  title={Modeling epsilon Eridani and its oscillations},
  author={David R. Soderblom and Werner Dappen},
  year={1989}
}
Models of the structure of the K2 V star Epsilon Eridani which are based on star luminosity, temperature, composition, age, and mixing-length parameter (alpha) are discussed. Comparisons are made with models proposed by Guenther and Demarque (1986) and Guenther (1987). Predicted oscillation frequencies are presented. 44 refs. 

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