Does the i-process operate at nearly solar metallicity?
- Details
- Published on 31 August 2023
Vol. 677
8. Stellar atmospheres
Does the i-process operate at nearly solar metallicity?
This paper presents a high-resolution spectroscopic analysis of 15 s-process rich candidates with close-to-solar metallicity. The authors found that two stars of their sample are enriched in both r- and s-process elements, with an abundance pattern compatible with i-process nucleosynthesis which is efficient in polluting asymptotic giant branch (AGB) star companions. If the i process is indeed active in objects such as AGB stars with a close-to-solar metallicity, an important impact on nucleosynthesis and galactic chemical evolution can be expected. In particular, the i-process contribution to our Solar System would need to be revisited.