New determinations of the chemical composition of Wolf-Rayet stars
The formation of the lines of ions He, H, N and C in the WR stars of different spectral subtypes has been studied using clumped wind models. Our new results agree well with the previous results obtained with smooth wind codes which make use of highly excited lines of different ions.
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| Veröffentlicht in: | Symposium - International Astronomical Union 1995, Vol.163, p.162-163 |
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| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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| Zusammenfassung: | The formation of the lines of ions He, H, N and C in the WR stars of different spectral subtypes has been studied using clumped wind models. Our new results agree well with the previous results obtained with smooth wind codes which make use of highly excited lines of different ions. |
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| ISSN: | 0074-1809 |
| DOI: | 10.1017/S0074180900201861 |