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

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

Description

Keywords

Citation

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