Observing solar-like oscillations

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dc.creatorKjeldsen, Hans
dc.creatorBedding, Timothy R.
dc.date1997-04-04
dc.date.accessioned2026-07-07T02:23:08Z
dc.date.available2026-07-07T02:23:08Z
dc.descriptionWe 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.
dc.descriptionTo appear in Proc. IAU Symposium 189, "Fundamental Stellar Properties: The Interaction between Observation and Theory", edited by T. R. Bedding, A. J. Booth and J. Davis (Kluwer: Dordrecht)
dc.identifierhttps://arxiv.org/abs/astro-ph/9704045
dc.identifierhttp://arxiv.org/abs/astro-ph/9704045
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11137
dc.subjectAstrophysics
dc.titleObserving solar-like oscillations
dc.typetext

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