New results on ground-based asteroseismology of solar-like stars

Details New results on ground-based asteroseismology of solar-like stars New results on ground-based asteroseismology of solar-like stars

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..505b&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Computer Science

Sound

Scientific paper

Observing stellar oscillations provides a powerful probe for studying stellar interiors. The frequencies of these modes depend on the properties of the star, such as sound speed, density, and rotation. The five-minute oscillations in the Sun, induced by stochastic excitation of its convective zone, have provided a wealth of information about the solar interior and has led to significant revisions to solar models. Recently, thanks to high precision Doppler measurements, solar-like oscillations have been clearly detected in a growing list of main sequence and subgiant stars. New results and prospects in this field are presented.

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