Abundance analysis of chemically peculiar stars in IC 4665. II. HD 161480

Atmospheric parameters and chemical abundances of HD 161480 were determined by means of spectrograms of 16.9 Å/mm of dispersion, using model atmosphere which include blanketing of several spectral lines and oscillator strength modern values. Overabundance of C II and some elements of Fe-group was fo...

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Guardado en:
Detalles Bibliográficos
Autor principal: Gargiulo, M.V.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1988
Materias:
Astronomía
Galaxia
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/142575
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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