Chemical similarities between the Galactic bulge and local thick disk red giant stars: analysis from optical data

被引:0
|
作者
Alves-Brito, Alan [1 ]
Melendez, Jorge [2 ]
Asplund, Martin [3 ]
机构
[1] Univ Sao Paulo, IAG, Sao Paulo, Brazil
[2] Univ Porto, Ctr Astrofis, Porto, Portugal
[3] Max Planck Inst Astrophys, Garching, Germany
来源
CHEMICAL ABUNDANCES IN THE UNIVERSE: CONNECTING FIRST STARS TO PLANETS | 2010年 / 265期
基金
巴西圣保罗研究基金会;
关键词
stars: abundances; Galaxy: bulge; Galaxy: disk; ABUNDANCE ANALYSIS; HIGH-RESOLUTION; EVOLUTION; SPECTRA;
D O I
10.1017/S1743921310000839
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Galactic structure and composition remain as one of the greatest open problems in modern astrophysics. We show here that there are chemical similarities between the Galactic bulge and local thick disk red giant stars. This finding puts strong constraints on the IMF, SFR. and chemical enrichment timescale of the bulge and thick disk. Our results are based upon a detailed elemental abundance analysis of 80 high S/N and high resolution optical spectra of giant stars, in the range -1.5 < [Fe/H] < +0.5.
引用
收藏
页码:342 / +
页数:2
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