Published April 4, 2022
| Version 1.1.1
Dataset
Open
Weak s-process
Authors/Creators
- 1. Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Eötvös Loránd Research Network (ELKH), Konkoly Thege M. út 15-17, 1121 Budapest, Hungary
- 2. Astrophysics Group, Faculty of Natural Sciences, Keele University, Keele ST5 5BG, UK
Description
Collection of certified trajectories, covering a wide range of weak s-process conditions. Every trajectory comes with the selected initial abundances and other key information, such as the reference of the publication, the stellar region from where it was extracted, the mass of the star and its metallicity.
FREQUENTLY ASKED QUESTIONS
Q: Can I use these trajectories for nuclear sensitivity studies and/or to compute ejected stellar yields?
A: These trajectories can be used for nuclear sensitivity studies, but they cannot be used to compute stellar yields.