ELEMENTAL ABUNDANCE ANALYSES WITH DAO SPECTROGRAMS .9. THE METALLIC-LINED STARS 15-VULPECULAE AND 32-AQUARII

被引：12

作者：

BOLCAL, C

KOCER, D

ADELMAN, SJ

机构：

[1] ISTANBUL UNIV OBSERV,CTR RES & APPL,ISTANBUL,TURKEY

[2] THE CITADEL,DEPT PHYS,CHARLESTON,SC 29409

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1992年 / 258卷 / 02期

关键词：

LINE PROFILES; STARS ABUNDANCES; STARS FUNDAMENTAL PARAMETERS; STARS INDIVIDUAL 15-VUL; STARS INDIVIDUAL 32-AQR;

D O I：

10.1093/mnras/258.2.270

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Following from previous papers of this study we present elemental abundance analyses of the sharp-lined bright Am stars 15 Vul and 32 Aqr. The values derived using fine analysis techniques are found using the stellar parameters, effective temperature and surface gravity, determined using optical-region spectrophotometry and Balmer line profiles as well as with the procedures of Moon & Dworetsky and of Lane & Lester. The latter star is a more extreme Am star than the former star. We also discuss possible ways to improve these analyses.

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页码：270 / 276

页数：7

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