Rubidium-rich Asymptotic Giant Branch Stars in the Magellanic Clouds
The Magellanic Clouds (MCs) offer a unique opportunity to study the stellar evolution and nucleosynthesis of massive Asymptotic Giant Branch (AGB) stars in low metallicity environments where distances are known. Rubidium is a key element to distinguish between high mass AGB stars and low mass AGB stars or other types of astronomical objects such as
García-Hernández, D. A.
Advertised on:
9
2011