Asteroseismology of subgiants and red giants

Details Asteroseismology of subgiants and red giants Asteroseismology of subgiants and red giants

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..17e..23k&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

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Scientific paper

Theoretical calculations show that one should expect subgiants and giants in the cooler part of the HR-Diagram to oscillate in a rich p-mode spectrum - like the one we find in the Sun and other solar-like stars. There have been a number of claimed detections of those oscillations, however, a number of challenges are making those stars somewhat difficult targets concerning unambiguous detection of "solar-like" oscillations. I will review the present status of asteroseismology of those stars and give examples of how one may progress further towards detection of a large number of oscillation frequencies in a large number of targets.

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