The slope of the RR Lyrae Mν-[Fe/H] relation

被引：48

作者：

Fernley, J

Carney, BW

Skillen, I

Cacciari, C

Janes, K

机构：

[1] IUE Observ, Madrid 28080, Spain

[2] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA

[3] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[4] Boston Univ, Dept Astron, Boston, MA 02215 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1998年 / 293卷 / 03期

关键词：

stars; variables; other; globular clusters; general;

D O I：

10.1046/j.1365-8711.1998.01309.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review the available observational data to show that the slope of the RR Lyrae M-V-[Fe/H] relation is 0.18 +/- 0.03. The recent claim by Feast that, because of biases, the true slope is much steeper is not justified.

引用

页码：L61 / L64

页数：4

共 18 条

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