The Sr-Y Abundance Peak in HR6127

Details The Sr-Y Abundance Peak in HR6127 The Sr-Y Abundance Peak in HR6127

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...104...80p&link_type=abstract

Astronomy and Astrophysics, Vol.104, P. 80, 1981

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

The relative elemental abundance in the Sr-Y-Zr peak on HR 6127 is the
only feature that contradicts the classification of this star as a cool
Ap. We show that using more appropriate gf-values the abundances of Y
and Zr are considerably reduced and become of the same order than those
observed in Am stars rather than in cool Ap stars.

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