Abundances of intermediate/low mass stars in the Galactic bulge

被引：2
作者：
Barbuy, B [1 ]
机构：
[1] Univ Sao Paulo, Fapesp, BR-01060970 Sao Paulo, Brazil
来源：
FROM EXTRASOLAR PLANETS TO COSMOLOGY: THE VLT OPENING SYMPOSIUM | 2000年
关键词：
D O I：
10.1007/10720961_53
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Detailed abundance analyses available for stars in the Galactic bulge are reviewed. These consist of 5 intermediate-mass stars in the Galactic center, 12 field stars in Baade's Window and a few stars in the bulge globular clusters NGC 6528 and NGC 6553. Clearly this is a field which will greatly benefit from the advent of high resolution spectroscopy with 8m class telescopes.
引用
收藏
页码：357 / 362
页数：6
相关论文
共 40 条
[1]  
Barbuy B, 1998, ASTRON ASTROPHYS, V333, P117
[2]  
BARBUY B, 1999, UNPUB
[3]  
Barbuy B., 1990, ESO C WORKSHOP P, V35, P83
[4]  
BARBUY B, 1999, IN PRESS GALAXY EVOL
[5]  
BARBUYB, 1999, ASTRON ASTROPHYS, V341, P539
[6]   Abundances for globular cluster giants .1. Homogeneous metallicities for 24 clusters [J].
Carretta, E ;
Gratton, RG .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 121 (01) :95-112
[7]   High-resolution abundance analysis of very metal-rich stars in the solar neighborhood [J].
Castro, S ;
Rich, RM ;
Grenon, M ;
Barbuy, B ;
McCarthy, JK .
ASTRONOMICAL JOURNAL, 1997, 114 (01) :376-387
[8]  
CATCHPOLE RM, 1999, IAU S, V192
[9]  
COHEN JG, 1999, UNPUB APJ
[10]  
Gratton RG, 1996, ASTRON ASTROPHYS, V314, P191
1234