Doppler ground-based asteroseismology of solar-like stars: results and prospects

Details Doppler ground-based asteroseismology of solar-like stars: results and prospects Doppler ground-based asteroseismology of solar-like stars: results and prospects

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..123b&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

Characterization of stellar oscillation modes allow to constrain theory of internal structure and evolution of stars. Recent improvements in radial velocity measurements have led to p-mode detections on some bright solar-type stars. We review some current and future ground-based programs and present some new results. These programs are compared to the future space missions.

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