NTT V, I colour-magnitude diagrams of the bulge globular cluster Tonantzintla 2

被引:15
作者
Bica, E
Ortolani, S
Barbuy, B
机构
[1] UNIV SAO PAULO,IAG,DEPT ASTRON,BR-01065970 SAO PAULO,BRAZIL
[2] UNIV FED RIO GRANDE SUL,DEPT ASTRON,BR-91500970 PORTO ALEGRE,RS,BRAZIL
[3] UNIV PADUA,DEPT ASTRON,I-35123 PADUA,ITALY
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1996年 / 120卷 / 01期
关键词
globular clusters; Ton; 2; HR diagram;
D O I
10.1051/aas:1996281
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Ton 2 is among the less-known Galactic globular clusters. We present for the first time colour magnitude diagrams in the V, I bands. We used the ESO NTT telescope under an excellent seeing of 0.6 ''. The horizontal branch is red and close to the red giant branch, tilted by some differential reddening. The horizontal branch morphology and the red giant branch curvature suggest a metallicity similar to that of 47 Tucanae. We derive a reddening of E(B - V) = 1.26 and a distance d. = 6.4 kpc. Therefore, Ton 2 is approximate to 2.0 kpc from the Galactic center, and it appears to belong to the bulge population, being however only moderately metal rich.
引用
收藏
页码:153 / 156
页数:4
相关论文
共 11 条
[1]  
BICA E, 1994, ASTRON ASTROPHYS SUP, V106, P161
[2]   REDDENINGS OF CEPHEIDS USING BVI PHOTOMETRY [J].
DEAN, JF ;
WARREN, PR ;
COUSINS, AWJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1978, 183 (03) :569-583
[3]  
Ortolani S, 1996, ASTRON ASTROPHYS, V306, P134
[4]  
ORTOLANI S, 1991, ASTRON ASTROPHYS, V249, pL31
[5]   NEAR-COEVAL FORMATION OF THE GALACTIC BULGE AND HALO INFERRED FROM GLOBULAR-CLUSTER AGES [J].
ORTOLANI, S ;
RENZINI, A ;
GILMOZZI, R ;
MARCONI, G ;
BARBUY, B ;
BICA, E ;
RICH, RM .
NATURE, 1995, 377 (6551) :701-704
[6]  
Ortolani S, 1996, ASTRON ASTROPHYS, V308, P733
[7]  
PISMIS P, 1959, B OBS TONANTZINTAL T, V18, P37
[8]  
REID MJ, 1993, ANNU REV ASTRON ASTR, V31, P345
[9]   CATALOG OF GALACTIC GLOBULAR-CLUSTER SURFACE-BRIGHTNESS PROFILES [J].
TRAGER, SC ;
KING, IR ;
DJORGOVSKI, S .
ASTRONOMICAL JOURNAL, 1995, 109 (01) :218-241
[10]  
WEBBINK RF, 1985, IAU S, V113, P541