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HD 27962, also known as 68 Tauri, is a Chemically Peculiar Am star member ofthe Hyades Open Cluster in the local arm of the Galaxy. We have modeled thehigh resolution SOPHIE (R=75000) spectrum of 68 Tauri using updated modelatmosphere and spectrum synthesis to derive chemical abundances in itsatmosphere. In particular, we have studied the effect of the inclusion ofHyperfine Structure of various Baryum isotopes on the determination of theBaryum abundance in 68 Tauri. We have also derived new abundances using updatedaccurate atomic parameters retrieved from the NIST database.

Hyperfine Structure and Abundances of Heavy Elements in 68 Tauri (HD 27962)