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The impact of updated Zr neutron-capture cross sections and new asymptotic giant branch models on our understanding of the S process and the origin of stardust

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Date

2014

Authors

Lugaro, Maria
Tagliente, G
Karakas, Amanda
Milazzo, P M
Kappeler, F
Davis, Andrew M
Savina, Michael R.

Journal Title

Journal ISSN

Volume Title

Publisher

IOP Publishing

Abstract

We present model predictions for the Zr isotopic ratios produced by slow neutron captures in C-rich asymptotic giant branch (AGB) stars of masses 1.25-4 M⊙ and metallicities Z = 0.01-0.03, and compare them to data from single meteoritic stardust silicon

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Keywords

Citation

URI

http://hdl.handle.net/1885/77322

Collections

ANU Research Publications

Source

Astrophysical Journal, The

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1088/0004-637X/780/1/95

Restricted until

2037-12-31

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01_Lugaro_The_impact_of_updated_Zr_2014.pdf (855.82 KB)

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