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Structure of Procyon A by a seismological approach
Published online by Cambridge University Press: 13 May 2016
Abstract
We consider the theoretical prediction of the power spectrum of oscillations of Procyon A, a bright subgiant star which shows solar like pulsations, comparing models computed by taking into account overshoot from the convective core, as well as diffusion of helium and heavy elements.
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- Session I: Global Structure and Evolution of the Solar Interior
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- Copyright © Astronomical Society of the Pacific 2001
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