The distance to the Fornax dwarf galaxy using red clump stars and the discrepancy between red clump and tip of the red giant branch distances

被引:26
作者
Bersier, D [1 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
基金
美国国家科学基金会;
关键词
galaxies : distances and redshifts; galaxies; individual; (Carina; Fornax; Large Magellanic Cloud); stars : late-type;
D O I
10.1086/318170
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I determine a distance to the Fornax dwarf galaxy using stars in the red clump and at the tip of the red giant branch. They are in very good agreement, with mu (0) = 20.66 mag. Comparing the magnitudes of the tip of the red giant branch and of the red clump in Fornax, Carina, and the Magellanic Clouds, I propose a possible solution to the problem of the discrepancy between these two types of distance measurements.
引用
收藏
页码:L23 / L26
页数:4
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