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Chemical abundance analysis of red giant branch stars in the globular cluster E3

Chemical abundance analysis of red giant branch stars in the globular cluster E3

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073371874

Chemical abundance analysis of red giant branch stars in the globular cluster E3

About this item

Full title

Chemical abundance analysis of red giant branch stars in the globular cluster E3

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2018-06

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Context. Globular clusters are known to host multiple stellar populations, which are a signature of their formation process. The globular cluster E3 is one of the few low-mass globulars that is thought not to host multiple populations. Aims. We investigate red giant branch stars in E3 with the aim of providing a first detailed chemical inventory fo...

Alternative Titles

Full title

Chemical abundance analysis of red giant branch stars in the globular cluster E3

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2073371874

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073371874

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1806.03327

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