Chemical abundances in bright giants of the globular cluster M62 (NGC 6266)
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Yong, David
Alves-Brito, Alan
Da Costa, Gary
Alonso-Garcia, Javier
Karakas, Amanda
Pignatari, Marco
Roederer, Ian U.
Aoki, Wako
Fishlock, Cherie
Grundahl, Frank
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Blackwell Publishing Ltd
Abstract
With the exception of Terzan 5, all the Galactic globular clusters that possess significant metallicity spreads, such as ω Cen and M22, are preferentially the more luminous clusters with extended horizontal branches. Here we present radial velocities and
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Monthly Notices of the Royal Astronomical Society
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Open Access
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