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Astron. Astrophys. Suppl. Ser. 137, 227-232

Elemental abundance studies of CP stars

II. The silicon stars HD 133029 and HD 192913[*]

Z. López-García1[*] - S.J. Adelman2

Send offprint request: S.J. Adelman

1 - Observatorio Astronómico "Felix Aguilar'', Universidad Nacional de San Juan, Argentina
2 - Department of Physics, The Citadel, 171 Moultrie Street, Charleston SC 29409, U.S.A.

Received November 2, 1998; accepted January 14, 1999


Fine analyses of the silicon stars HD 133029 and HD 192913 are presented using ATLAS9 model atmospheres whose predictions fit the optical region spectrophotometry and H$\gamma$ profiles and have the same bulk metallicity as the deduced abundances. Both are very He poor stars. The light elements are mostly solar except for silicon, and all the heavier elements, except nickel in HD 133029 which is solar, are greatly overabundant. The iron peak elements are typically 10 times overabundant. SrYZr are of order of 100 times solar. The rare earths are 1000 or more times overabundant.

Key words: stars: chemically peculiar -- stars: abundances -- stars: individual: HD 133029 -- stars: individual: HD 192913

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