Red Giants as Asteroseismology Targets

Details Red Giants as Asteroseismology Targets Red Giants as Asteroseismology Targets

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..349..305m&link_type=abstract

Astrophysics of Variable Stars, Pecs, Hungary, 5-10 September 2005, Sterken, C. and Aerts, C. (eds). ASP Conference Series, Vol.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The red giant region in the H-R diagram can be occupied by stars in the hydrogen-shell burning phase as well as stars in the helium-burning phase. We have studied the evolution of a 3 ~ M&sun; star in these two phases. The helium-burning phase can give rise to the development a of semi-convective region. We study the implications of the lack of an adequated semi-convective treatment and we present preliminary results on the oscillation properties of the stellar models in the red giant phase.

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