An age difference of two billion years between a metal-rich and a metal-poor globular cluster

Date

Authors

Hansen, B M S
Kalirai, Jason S
Anderson, Jay
Dotter, Aaron
Richer, Harvey B
Rich, R M
Shara, Michael M
Fahlman, Gregory G
Hurley, Jarrod
King, I R

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Macmillan Publishers Ltd

Abstract

Globular clusters trace the formation history of the spheroidal components of our Galaxy and other galaxies, which represent the bulk of star formation over the history of the Universe. The clusters exhibit a range of metallicities (abundances of elements

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Source

Nature

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Restricted until

2037-12-31