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CESAM Solar Models
Published online by Cambridge University Press: 12 April 2016
Abstract
Solar models have been computed using the code CESAM constructed at Nice (Morel, 1992), and the new opacities of Livermore for different mixtures. Their global characteristics, predicted capture rates of neutrinos for the chlorine and gallium experiments and their seismological properties are given.
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- I. Setting the stage: Sun, Stars Galaxies and the Universe
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- Copyright © Astronomical Society of the Pacific 1993