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CESAM Solar Models

Published online by Cambridge University Press:  12 April 2016

P. Morel,
G. Berthomieu,
J. Provost and
Y. Lebreton
P. Morel
Affiliation:
Cassini, URA CNRS 1362, Observatoire de la Côte d’Azur, Nice
G. Berthomieu
Affiliation:
Cassini, URA CNRS 1362, Observatoire de la Côte d’Azur, Nice
J. Provost
Affiliation:
Cassini, URA CNRS 1362, Observatoire de la Côte d’Azur, Nice
Y. Lebreton
Affiliation:
DASGAL, URA CNRS 335, Observatoire de Paris, Paris

Abstract

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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.

Information

Type
I. Setting the stage: Sun, Stars Galaxies and the Universe
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993, pp. 54 - 56
Copyright
Copyright © Astronomical Society of the Pacific 1993

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