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Precise and accurate interpolated stellar oscillation frequencies on the main sequence

Published online by Cambridge University Press:  18 February 2014

Warrick H. Ball
Affiliation:
Institut für Astrophysik, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany email: [email protected] Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
Jesper Schou
Affiliation:
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
Laurent Gizon
Affiliation:
Institut für Astrophysik, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany email: [email protected] Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
João P. C. Marques
Affiliation:
Institut für Astrophysik, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany email: [email protected]
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Abstract

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High-quality data from space-based observatories present an opportunity to fit stellar models to observations of individually-identified oscillation frequencies, not just the large and small frequency separations. But such fits require the evaluation of a large number of accurate stellar models, which remains expensive. Here, we show that global-mode oscillation frequencies interpolated in a grid of stellar models are precise and accurate, at least in the neighbourhood of a solar model.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Christensen-Dalsgaard, J. 2008, Ap&SS, 316, 113Google Scholar
Kallinger, T., Gruberbauer, M., Guenther, D. B., Fossati, L., & Weiss, W. W. 2010, A&A, 510, A106Google Scholar
Marques, J. P., Goupil, M.-J., Lebreton, Y., et al. 2013, A&A, 549, A74Google Scholar