Observing solar-like oscillations

Preprint

4 April 1997

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9704045

Abstract

We review techniques for measuring stellar oscillations in solar-type stars. Despite great efforts, no unambiguous detections have been made. A new method, based on monitoring the equivalent widths of strong lines, shows promise but is yet to be confirmed. We also discuss several subtleties, such as the need to correct for CCD non-linearities and the importance of data weighting.

Keywords

TECHNIQUES FOR MEASURING
STELLAR OSCILLATIONS
LIKE OSCILLATIONS
REVIEW TECHNIQUES
MEASURING STELLAR
OBSERVING SOLAR
SOLAR LIKE
STARS

All Related Versions

Version 1, 1997-04-04, ArXiv

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