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On the issue of surface-related problems in stellar parameter estimation
Published online by Cambridge University Press: 19 December 2013
Abstract
I address the problem of estimating stellar parameters using asteroseismic data. In particular I focus on the biases introduced the differences existing between observed and theoretical oscillation frequencies introduced by a poor modelling of near-surface layers. I review some methods to evaluate this shift and discuss briefly some studies trying to take into account this effect while estimating stellar parameters.
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- Research Article
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- © EAS, EDP Sciences, 2013
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