Effect of microscopic diffusion on asteroseismic properties of intermediate-mass stars

Details Effect of microscopic diffusion on asteroseismic properties of intermediate-mass stars Effect of microscopic diffusion on asteroseismic properties of intermediate-mass stars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...432..225p&link_type=abstract

Astronomy and Astrophysics, Volume 432, Issue 1, March II 2005, pp.225-233

Astronomy and Astrophysics

Astrophysics

7

Stars: Oscillations, Stars: Evolution, Stars: Oscillation, Diffusion

Scientific paper

Results on the effects of microscopic diffusion on the modeling and oscillations of
solar-like stars are discussed. Comparisons between models with and without microscopic diffusion, subjected to observational constraints, namely effective temperature, luminosity, surface metallicity and mass
derived from photometry, spectroscopy and astrometry, are presented. We point out and discuss a signature of microscopic diffusion on the oscillation frequencies.

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