Título alternativo:Abundance analysis of chemically peculiar stars in IC 4665. II. HD 161480
Resumen
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 found. Results were compared with those obtained for normal B stars and other stars of the group. This paper will be published in Astrophysical Letters and Communications.
Información general
Fecha de publicación:1988
Idioma del documento:Español
Revista:Boletín de la Asociación Argentina de Astronomía; no. 34
Institución de origen:Asociación Argentina de Astronomía
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