Sodium content as a predictor of the advanced evolution of globular cluster stars
Date
Authors
Campbell, Simon W
D’Orazi , V
Yong, David
Constantino, Thomas N
Lattanzio, John
Stancliffe, Richard
Angelou, G C
Wylie de Boer, Elizabeth
Grundahl, Frank
Journal Title
Journal ISSN
Volume Title
Publisher
Macmillan Publishers Ltd
Abstract
The asymptotic giant branch (AGB) phase is the final stage of nuclear burning for low-mass stars. Although Milky Way globular clusters are now known to harbour (at least) two generations of stars, they still provide relatively homogeneous samples of stars
Description
Citation
Collections
Source
Nature
Type
Book Title
Entity type
Access Statement
License Rights
Restricted until
2037-12-31