Oscillations in solar-type stars: recent observational results

Details Oscillations in solar-type stars: recent observational results Oscillations in solar-type stars: recent observational results

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..17e..22b&link_type=abstract

Highlights of Recent Progress in the Seismology of the Sun and Sun-Like Stars, 26th meeting of the IAU, Joint Discussion 17, 23

Physics

Scientific paper

The past few years have seen a breakthrough in observing oscillations in solar-type stars. We now have moved from ambiguous detections to firm measurements, and there are now several stars for which numerous oscillation frequencies have been measured. I will review the recent results from high-precision Doppler measurements on stars such as α Centauri A and B, τ Ceti and the planet-hosting star μ Arae. Asteroseismology has moved from dream to reality and the prospects are very exciting.

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