THE STRUCTURE OF THE CORE OF 47-TUCANAE FROM HUBBLE-SPACE-TELESCOPE OBSERVATIONS

被引:35
作者
DEMARCHI, G
PARESCE, F
FERRARO, FR
机构
[1] OSSERVATORIO ASTRON BOLOGNA,I-40126 BOLOGNA,ITALY
[2] UNIV FLORENCE,DIPARTIMENTO ASTRON,I-50121 FLORENCE,ITALY
关键词
GLOBULAR CLUSTERS; INDIVIDUAL; (47-TUC); HERTSPRUNG-RUSSELL DIAGRAM; STARS; LUMINOSITY FUNCTION; MASS FUNCTION; TECHNIQUES; IMAGE PROCESSING;
D O I
10.1086/191766
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A set of moderately deep. high-resolution images of the core of the Galactic globular cluster NGC 104 (47 Tucanae) taken by the Faint Object Camera F/48 relay on the Hubble Space Telescope through the filters F140W, F220W, and F342W are presented and analyzed. The core is completely resolved in these bands for the first time, with approximately 3500 stars reliably detected and measured in the 44'' x 44'' F342W frame down to instrumental magnitude m342 congruent-to 19.5. These images are used to derive color magnitude diagrams that extend and confirm the discovery of a population of about 20 blue stragglers in the cluster core. The luminosity function of the brightest stars (AGB, HB, RGB, and SGB) shows that the sample is 99% complete at m342 congruent-to 16. down to 61% at m342 congruent-to 18.
引用
收藏
页码:293 / 314
页数:22
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