Abundances of the rare earths in the sun

N. Grevesse, G. Blanquet

Research output: Contribution to journalArticle

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.
LanguageEnglish
Pages5-17
Number of pages13
JournalSolar Physics
Volume8
Issue number1
DOIs
StatePublished - 1 Jul 1969

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sun
rare earth elements
solar spectra
meteorites
tracing
nuclear fusion
Switzerland
meteorite
stations
high resolution
station

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Grevesse, N. ; Blanquet, G./ Abundances of the rare earths in the sun. In: Solar Physics. 1969 ; Vol. 8, No. 1. pp. 5-17
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Abundances of the rare earths in the sun. / Grevesse, N.; Blanquet, G.

In: Solar Physics, Vol. 8, No. 1, 01.07.1969, p. 5-17.

Research output: Contribution to journalArticle

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AU - Grevesse,N.

AU - Blanquet,G.

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PY - 1969/7/1

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Grevesse N, Blanquet G. Abundances of the rare earths in the sun. Solar Physics. 1969 Jul 1;8(1):5-17. Available from, DOI: 10.1007/BF00150651