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

被引：33

作者：

Caliskan, H ^{[1
]}

Adelman, SJ ^{[1
]}

机构：

[1] THE CITADEL, DEPT PHYS, CHARLESTON, SC 29409 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1997年 / 288卷 / 02期

关键词：

stars; abundances; individual; 2; Lyn; omega UMa stars; theta Aql;

D O I：

10.1093/mnras/288.2.501

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：501 / 511

页数：11

共 57 条

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