Abundances of the rare earths in the sun

N. Grevesse; G. Blanquet

doi:10.1007/BF00150651

Abundances of the rare earths in the sun

N. Grevesse, G. Blanquet

Résultats de recherche: Contribution à un journal/une revue › Article › Revue par des pairs

Résumé

We have determined the solar abundances of the rare earths (La, Ce, Pr, Nd, Sm, Eu, Gd, Dy, Er, Tm, Yb, Lu) on the basis of measurements made on new high-resolution tracings of the solar spectrum obtained at the International Scientific Station of the Jungfraujoch (Switzerland) by L. Delbouille, L. Neven and G. Roland. Our results (Table XV) are compared with those of other authors for the sun and meteorites as well as with the abundances predicted by nucleosynthesis theories.

langue originale	Anglais
Pages (de - à)	5-17
Nombre de pages	13
journal	Solar Physics
Volume	8
Numéro de publication	1
Les DOIs	https://doi.org/10.1007/BF00150651
Etat de la publication	Publié - 1 juil. 1969

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10.1007/BF00150651

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title = "Abundances of the rare earths in the sun",

abstract = "We have determined the solar abundances of the rare earths (La, Ce, Pr, Nd, Sm, Eu, Gd, Dy, Er, Tm, Yb, Lu) on the basis of measurements made on new high-resolution tracings of the solar spectrum obtained at the International Scientific Station of the Jungfraujoch (Switzerland) by L. Delbouille, L. Neven and G. Roland. Our results (Table XV) are compared with those of other authors for the sun and meteorites as well as with the abundances predicted by nucleosynthesis theories.",

author = "N. Grevesse and G. Blanquet",

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AU - Blanquet, G.

PY - 1969/7/1

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N2 - We have determined the solar abundances of the rare earths (La, Ce, Pr, Nd, Sm, Eu, Gd, Dy, Er, Tm, Yb, Lu) on the basis of measurements made on new high-resolution tracings of the solar spectrum obtained at the International Scientific Station of the Jungfraujoch (Switzerland) by L. Delbouille, L. Neven and G. Roland. Our results (Table XV) are compared with those of other authors for the sun and meteorites as well as with the abundances predicted by nucleosynthesis theories.

AB - We have determined the solar abundances of the rare earths (La, Ce, Pr, Nd, Sm, Eu, Gd, Dy, Er, Tm, Yb, Lu) on the basis of measurements made on new high-resolution tracings of the solar spectrum obtained at the International Scientific Station of the Jungfraujoch (Switzerland) by L. Delbouille, L. Neven and G. Roland. Our results (Table XV) are compared with those of other authors for the sun and meteorites as well as with the abundances predicted by nucleosynthesis theories.

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Abundances of the rare earths in the sun

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