Elemental abundance study of the CP star HD 206653

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 over...

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Detalles Bibliográficos
Autores: Albacete-Colombo, J.F., López-García, Z., Levato, H., Malaroda, S.M., Grosso, M.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2002
País:Argentina
Institución:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
Repositorio:Biblioteca Digital (UBA-FCEN)
Idioma:inglés
OAI Identifier:paperaa:paper_00046361_v392_n2_p613_AlbaceteColombo
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v392_n2_p613_AlbaceteColombo
Access Level:acceso abierto
Palabra clave:Stars: abundances
Stars: chemically peculiar
Stars: individual: HD 206653
Airborne telescopes
Cerium
Europium
Mathematical models
Rare earths
Silicon
Solar system
Iron peak elements
Light elements
Stars
Astrophysics
Descripción
Sumario: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.