Modeling Epsilon Eridani and its oscillations

Details Modeling Epsilon Eridani and its oscillations Modeling Epsilon Eridani and its oscillations

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342..945s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 342, July 15, 1989, p. 945-950.

Astronomy and Astrophysics

Astrophysics

30

Late Stars, Stellar Models, Stellar Oscillations, Abundance, Helium, Metallicity, Stellar Evolution, Stellar Luminosity, Stellar Temperature

Scientific paper

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.

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