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Space and Ground Based Data for Asteroseismology

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Abstract

Measuring eigenfrequencies and identifying eigenmodes provide the observational basis for a significant improvement in our understanding of stellar evolution and structure.Development throughout the last few years show that we may be at the dawn of a `Golden Age'for Asteroseismology. For this to become a reality we only need two things:Better data and better models. In this paper I describe some aspectsof how one detects stellar oscillations.

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Authors and Affiliations

  1. Institut for Fysik og Astronomi, Aarhus Universitet, Denmark

    H. Kjeldsen

  2. Teoretisk Astrofysik Center, Danmarks Grundforskningsfond, Denmark

    H. Kjeldsen

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  1. H. Kjeldsen
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Kjeldsen, H. Space and Ground Based Data for Asteroseismology. Astrophysics and Space Science 284, 1–12 (2003). https://doi.org/10.1023/A:1023287206563

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  • DOI: https://doi.org/10.1023/A:1023287206563

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