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The Color-Magnitude Relation for Metal-Poor...
Preprint

The Color-Magnitude Relation for Metal-Poor Globular Clusters in M87: Confirmation From Deep HST/ACS Imaging

Abstract

Metal-poor globular clusters (GCs) are our local link to the earliest epochs of star formation and galaxy building. Studies of extragalactic GC systems

Authors

Peng EW; Jordan A; Blakeslee JP; Mieske S; Cote P; Ferrarese L; Harris WE; Madrid JP; Meurer GR

Publication date

July 15, 2009

DOI

10.48550/arxiv.0907.2524

Preprint server

arXiv

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