The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints (2019)
Attributed to:
Astrophysics at The University of Hull
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1908.09160
Publication URI: https://arxiv.org/abs/1908.09160
Type: Other