Abundance anomalies in AP stars and the noble gas structure

Details Abundance anomalies in AP stars and the noble gas structure Abundance anomalies in AP stars and the noble gas structure

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apl....17....3c&link_type=abstract

Astrophysical Letters, vol. 17, no. 1, 1976, p. 3-5.

Astronomy and Astrophysics

Astrophysics

1

A Stars, Abundance, Gaseous Diffusion, Ionic Diffusion, Rare Gases, Cerium, Magnetic Stars, Stellar Spectra, Xenon, Yttrium

Scientific paper

A simple diffusion hypothesis is tested in which the noble-gas structure
of diffusing ions is the dominant factor. The hypothesis fails to
predict large overabundances of yttrium and cerium, but shows promise in
predicting the lighter lanthanides in many Ap stars.

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