The distance to the M31 globular cluster system

被引：115

作者：

Holland, S ^{[1
]}

机构：

[1] Aarhus Univ, Inst Fys & Astronomi, DK-8000 Aarhus C, Denmark

来源：

ASTRONOMICAL JOURNAL | 1998年 / 115卷 / 05期

关键词：

galaxies; distances and redshifts; individual; (M31); star clusters;

D O I：

10.1086/300348

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The distance to the centroid of the M31 globular cluster system is determined by fitting theoretical isochrones to the observed red giant branches of 14 globular clusters in M31. The mean true distance modulus of the M31 globular clusters is found to be mu(0) = 24.47 +/- 0.07. This is consistent with distance moduli for M31 that have been obtained using other distance indicators.

引用

页码：1916 / 1920

页数：5

共 26 条

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