Epsilon Eridani revisited

Details Epsilon Eridani revisited Epsilon Eridani revisited

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..653d&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 653-655 (SEE N89-25819 19-92)

Physics

Stellar Interiors, Stellar Luminosity, Stellar Oscillations, Stellar Physics, P Waves, Stellar Evolution, Stellar Models

Scientific paper

In the light of the unsatisfactory theoretical explanation of the observed p-mode frequency separation of epsilon Eri of 172 microHz, and of the fact that the seismological observation is not confirmed, a series of models was computed. Only the observational input available prior to the seismological determination is taken into account. Predictions for the p-mode frequency separation that lie between 198 and 244 microHz are obtained.

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