Energetic properties of stellar pulsation across the HR diagram
1 : Instytut Astronomiczny, Uniwersytet Wroclawski
(IAUWr)
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Website
The energetic properties of stellar pulsations depend on the internal structure of a star and excitation mechanism. One of the main uncertainties in pulsational computations are connected with the presence of convection, rotation or magnetic field as well as microscopic physics (e.g., opacities).
I will review types of modes which are observed in stars on various evolutionary stages. In particular, I will discuss energetic aspects of oscillation modes, i.e., excitation, distribution of kinetic energy and rotational kernel. Finally, I will try to answer the question: what can we learn from these properties about the stellar structure and input physics ?
| Subject : | : | invited |
| Topics | : | Session 1 - Probing stellar structure and evolution with asteroseismology |
| PDF version | : |  PDF version |
- Presentation
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