Elemental abundance analyses with DAO spectrograms .17. The superficially normal early A stars 2 Lyncis, omega Ursa Majoris and phi Aquilae

Caliskan, Hülya; ADELMAN, SJ

doi:10.1093/mnras/288.2.501

Elemental abundance analyses with DAO spectrograms .17. The superficially normal early A stars 2 Lyncis, omega Ursa Majoris and phi Aquilae

Atıf İçin Kopyala

Caliskan H., ADELMAN S.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.288, sa.2, ss.501-511, 1997 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 288 Sayı: 2
Basım Tarihi: 1997
Doi Numarası: 10.1093/mnras/288.2.501
Dergi Adı: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Sayfa Sayıları: ss.501-511
İstanbul Üniversitesi Adresli: Evet

Özet

Elemental abundances of the superficially normal early A stars 2 Lyn, omega UMa and phi Aql are derived consistent with previous studies in this series, using spectrograms obtained with Reticon and CCD detectors. The derived elemental abundances of 2 Lyn are usually very close to solar. Both omega UMa and phi Aql, which are considered to be hot metallic-line stars, show He underabundances as well as overabundances of many iron-peak and heavier elements.