7–13 Sept 2024
Asia/Shanghai timezone
The third circular has been released.

The Role of Carbon-Oxygen Shell Interactions in the Nucleosynthesis and Final Fate of Massive Stars

10 Sept 2024, 09:25
25m
Invited Talk Stellar Evolutions and Hydrostatic Burning Processes Stellar Evolutions and Hydrostatic Burning Processes

Speaker

Lorenzo ROBERTI (Konkoly Observatory, HUN-REN CSFK)

Description

Carbon-oxygen (C-O) shell interactions in the late evolutionary stages of massive stars play a crucial role in determining their final fate and have a significant impact on the pre-supernova and explosive nucleosynthesis. In this talk, I will explore the complex dynamics within C-O shells, and how these interactions drive the production of intermediate and heavy elements. Recent advancements in theoretical models and observational data provide new insights into how C-O shell interactions influence the synthesis of elements, shaping the chemical evolution of the star and the broader universe.

Primary author

Lorenzo ROBERTI (Konkoly Observatory, HUN-REN CSFK)

Presentation materials