Issue |
A&A
Volume 392, Number 2, September III 2002
|
|
---|---|---|
Page(s) | 613 - 617 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20020775 | |
Published online | 30 August 2002 |
Elemental abundance study of the CP star HD 206653
1
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, 1900 La Plata, Argentina
2
Complejo Astronómico El Leoncito, C.C 467, 5400 San Juan, Argentina
3
Member of the Carrera del Investigador Científico, CONICET, Consejo Nacional de Investigaciones Científicas y Técnicas de la República Argentina
4
Facultad de Ciencias Exactas, Físicas y Naturales, Universidad Nacional de San Juan, Argentina
5
Comisión de Investigaciones Científicas de la Provincia de Buenos Aires, Argentina
Corresponding author: H. Levato, hlevato@casleo.gov.ar
Received:
30
October
2001
Accepted:
11
April
2002
An analysis of the abundances of the Silicon star HD 206653 is presented using an ATLAS9 model atmosphere and observational material taken with a REOSC echelle spectrograph attached to the Jorge Sahade 2.15 m telescope at CASLEO. The light elements are solar or deficient except silicon which is overabundant by a factor of 5. The iron peak elements are all overabundant by factors between 10 and 50. Sr and Y are around 1000 times the solar values. Among the Rare Earths only Ce and Eu are identified; both are overabundant by large factors.
Key words: stars: chemically peculiar / stars: abundances / stars: individual: HD 206653
© ESO, 2002
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