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A Hertzsprung-Russell diagram for stellar oscillations

Published online by Cambridge University Press:  03 August 2017

Jørgen Christensen-Dalsgaard*
Affiliation:
Astronomisk Institut, Aarhus Universitet, DK-8000 Aarhus C, Denmark

Abstract

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I present evolutionary tracks and curves of constant central hydrogen abundance in diagrams based on frequencies of high-order, low-degree p modes. For stars with masses between 0.7 and 1.5 M, a clean separation is obtained between the effects of varying mass and varying evolutionary state.

Type
Chapter 4: Asteroseismology: Results and Prospects
Copyright
Copyright © Reidel 1988 

References

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