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The s-process in AGB stars

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Date

2010

Authors

Karakas, Amanda
Lugaro, Maria

Journal Title

Journal ISSN

Volume Title

Publisher

Conference Organising Committee

Abstract

About half of the solar abundances of elements heavier than iron are made by the slow neutron capture process (the s process) occurring in low and intermediate-mass asymptotic giant branch (AGB) stars. Elements are dredged from the core to the surface and

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Keywords

Citation

URI

http://hdl.handle.net/1885/84037

Collections

ANU Research Publications

Source

Proceedings of Science

Type

Conference paper

Book Title

Entity type

Access Statement

License Rights

DOI

Restricted until

2037-12-31

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