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| Paper: |
Red Giants as Asteroseismology Targets |
| Volume: |
349, Astrophysics of Variable Stars |
| Page: |
305 |
| Authors: |
Moreira, O. |
| Abstract: |
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 MSolar 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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