ELEMENTAL ABUNDANCE ANALYSES WITH DAO SPECTROGRAMS .8. THE NORMAL F-MAIN SEQUENCE STARS THETA-CYGNI AND IOTA PISCIUM
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, sa.3, ss.329-333, 1991 (SCI-Expanded)
- Yayın Türü: Makale / Tam Makale
- Basım Tarihi: 1991
- Doi Numarası: 10.1093/mnras/252.3.329
- Dergi Adı: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED)
- Sayfa Sayıları: ss.329-333
- Açık Arşiv Koleksiyonu: AVESİS Açık Erişim Koleksiyonu
- İstanbul Kültür Üniversitesi Adresli: Hayır
Özet
Elemental abundance analyses of the normal F dwarfs theta-Cygni and iota-Piscium are performed and found to be consistent with previous papers of this study. Our derived microturbulences of 1.5 and 1.0 km s-1 are slightly smaller than found by other recent investigations. The elemental abundances derived using fine analysis techniques are for the most part close to solar. Those which are not should be carefully re-examined using spectral synthesis techniques. The effects of small changes in the adopted effective temperatures and surface gravities are also presented.