Convective overshooting in the evolution and seismology of eta Bootis

Details Convective overshooting in the evolution and seismology of eta Bootis Convective overshooting in the evolution and seismology of eta Bootis

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...404..341d&link_type=abstract

Astronomy and Astrophysics, v.404, p.341-353 (2003)

Astronomy and Astrophysics

Astrophysics

42

Stars: Individual: Eta Bootis, Stars: Evolution, Stars: Oscillations

Scientific paper

In the near future frequencies of solar-like oscillation will be observed by the several planned space missions. In order to assess the information that will be available from such observations, we consider theoretical predictions of the frequency spectrum of oscillations of the star eta Bootis, which shows solar-type pulsations. We present results obtained by comparing ``classical'' evolution models with models computed by taking into account overshooting from the convective core.

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