arXiv · 1309.3044
Precise and accurate interpolated stellar oscillation frequencies on the main sequence
Abstract
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.
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Warrick H. Ball, Jesper Schou, Laurent Gizon, João P. Marques. 2013-09-12. Precise and accurate interpolated stellar oscillation frequencies on the main sequence. https://doi.org/10.1017/s1743921313014646
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