Elemental Abundances of Yttrium and Zirconium in the Mercury / Manganese Stars Phi-Herculis Kappa-Cancri and Iota-Coronae

Details Elemental Abundances of Yttrium and Zirconium in the Mercury / Manganese Stars Phi-Herculis Kappa-Cancri and Iota-Coronae Elemental Abundances of Yttrium and Zirconium in the Mercury / Manganese Stars Phi-Herculis Kappa-Cancri and Iota-Coronae

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...271..273r&link_type=abstract

Astronomy and Astrophysics, Vol.271, NO. 1/APRI, P. 273, 1993

Astronomy and Astrophysics

Astrophysics

2

Atomic Data, Stars: Abundances, Stars: Atmospheres, Stars: Chemically Peculiar

Scientific paper

The yttrium and zirconium abundances in the three mercury-manganese
stars φ-Herculis, κ-Cancri and ι-Coronae-Borealis are
derived from spectral lines of the third (doubly ionized) spectra.
Comparisons with results from previous analyses of second spectra
indicate a departure from the LTE ionization balance.

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