Physics of Solar-Like Oscillations

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The physics of solar and stellar oscillations determine their observable properties: frequencies amplitudes lifetimes line asymmetries and phase relations. In the solar case these quantities have been measured often with high precision and much has been learned about the properties of the solar interior and the properties of the oscillations. I discuss some examples of these inferences concentrating mostly on the low-degree modes for which corresponding information may be expected for distant stars. In addition I consider the current state of investigations of solar-like oscillations in other stars and the prospects for an improved understanding of the physics of such oscillations.

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