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...
Guardado en:
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1988
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/142575 |
| Aporte de: |
| Sumario: | 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. |
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