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Sodium content as a predictor of the advanced evolution of globular cluster stars

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Date

2013

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

Keywords

Keywords: sodium; cosmology; evolutionary theory; sodium; spectroscopy; timescale; article; asymptotic giant branch; chemical analysis; conceptual framework; cosmological phenomena; evolution; mathematical analysis; measurement; predictive value; priority journal;

Citation

URI

http://hdl.handle.net/1885/73011

Collections

ANU Research Publications

Source

Nature

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1038/nature12191

Restricted until

2037-12-31

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01_Campbell_Sodium_content_as_a_predictor_2013.pdf (400.49 KB)

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