arXiv · 0808.1889
On The Origin of the Blue Tilt in Extragalactic Globular Cluster Systems
Abstract
Some early-type galaxies show a correlation between color and integrated magnitude among the brighter metal-poor globular clusters (GCs). This phenomenon, known as the blue tilt, implies a mass-metallicity relationship among these clusters. In this paper we show that self-enrichment in GCs can explain several aspects of the blue tilt, and discuss predictions of this scenario.
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Jay Strader, Graeme Smith. 2008-08-13. On The Origin of the Blue Tilt in Extragalactic Globular Cluster Systems. https://doi.org/10.1088/0004-6256%2F136%2F5%2F1828
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